The galaxy exhibits an overall elliptical morphology. The light distribution appears centrally concentrated with a smooth profile, suggesting a relatively evolved system. However, there is evidence of some faint, extended features or tidal tails, which are indicative of possible past or ongoing interactions or merging events. The central region shows a yellowish hue, potentially indicating an older stellar population or a significant dust component. There's a noticeable extension or plume of light emanating from the central region towards one direction, which could be a result of tidal interactions or an active galactic nucleus jet.
