The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution with a concentrated central bulge. The light profile suggests an older stellar population, as indicated by the reddish-yellow hue dominating the galaxy's overall color. There is little evidence of spiral arm structure or significant dust lanes. The overall shape is roughly round, exhibiting a minor deviation from perfect circularity. No signs of active galactic nuclei or recent major merger events are readily apparent, although there might be minor tidal disturbances suggesting past gravitational interactions. The galaxy appears relatively isolated, with no nearby companions visibly interacting. The absence of bright, blue regions suggests a low current star formation rate.
