The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical-like profile, showing a high degree of circularity. There is no obvious presence of a distinct disk or spiral arm structure. A subtle color gradient is discernible, with the central region showing a slightly yellower hue, suggestive of an older stellar population, while the outer regions display a bluer tint which may point to younger stars or ongoing, but low level, star formation. There are no strong signs of tidal disturbances or interactions with other galaxies; however, it's possible there is a minor disturbance visible in the outer regions. The overall appearance suggests that this object is likely a massive galaxy that is relatively evolved.
