The galaxy presents a generally smooth and rounded morphology, though there are notable features suggestive of a complex structure. The central region exhibits a high concentration of light, appearing as a bright, somewhat diffuse core. Moving outward from the core, the light gradually diminishes. There's a hint of possible disk-like structure, but its definition is not sharp. The color profile seems to transition from a yellower hue in the central regions to a slightly bluer tone in the outer parts of the galaxy. There appears to be evidence of possible tidal interactions or merging events present in this galaxy. There are areas of distortion and asymmetry that would support the interaction hypothesis.
