The galaxy presents a generally smooth appearance, suggesting an elliptical or lenticular morphology. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades outwards. The overall color appears slightly redder, indicative of an older stellar population and lower star formation activity. The galaxy exhibits a mostly circular shape, with a slight elongation along one axis. There is no strong evidence of spiral arms or a prominent disk structure. No obvious signs of recent major mergers or strong tidal disturbances are observed, however, there is potentially a very minor distortion, it is difficult to determine.
