The galaxy presents a complex morphology, appearing to consist of two distinct components or objects in close proximity and apparent interaction.

The primary, more luminous component exhibits a relatively smooth, rounded profile. Its light is concentrated towards the center, appearing bright white with blue hues at the center. This may be due to a concentration of younger stars.

The secondary component presents a less defined, more diffuse appearance. The light emitted from this component is of a yellow hue, suggesting an older stellar population. There appears to be a possible tidal bridge or stream of material connecting the two components, indicating gravitational interaction. The overall structure appears to be undergoing a merging or interaction event, resulting in a disturbed morphology.
