The galaxy presents a primarily smooth, elliptical morphology. The primary light emission appears concentrated in a central bulge, exhibiting a yellowish hue, suggesting an older stellar population. There are subtle indications of features or a disk structure, potentially indicative of ongoing or past merging events. A secondary, brighter region with a bluer color is visible, slightly offset from the central bulge, which could be due to an active galactic nucleus or recent star formation activity. There appear to be signs of gravitational disturbance and tidal interactions, indicating ongoing or previous galaxy mergers. Overall, it shows a disturbed system of stars and potentially active regions with both old and possibly some younger stellar populations.
