The galaxy presents a complex morphology, exhibiting characteristics that suggest an ongoing or recent interaction or merging event. The core region appears primarily smooth, with a dominant central bulge that appears largely spheroidal. The light distribution indicates a relatively high concentration of older stellar populations within this central region, which likely contributes significantly to its overall luminosity, but does have some evidence of bluer light, indicating some pockets of star formation.

There is visual evidence for potential tidal features or distortions extending beyond the central region. A faint, diffuse halo surrounds the main body. Distinct components can be seen extending from the main bulge and surrounding halo, one of which has bluer light, which could be an arm or plume structure, suggesting ongoing interactions or mergers. The galaxy displays an irregular shape, not strictly elliptical or spiral, which may be indicative of a system in flux due to gravitational interactions. The colour gradients across the galaxy's structure indicate varying stellar populations and potentially differential dust extinction. Regions with bluer hues hint at recent star formation possibly triggered by the interaction event. The system does not have a clearly defined disk, but exhibits signs of recent interactions that could have disrupted any well-defined disk-like structure that could have previously existed.
