The galaxy appears to be an elliptical galaxy with a smooth, diffuse morphology. The central bulge is a bright, concentrated yellowish-white, gradually fading into the outer regions. There is no prominent spiral arm structure or distinct features, suggesting an older stellar population. The overall color of the galaxy has a slight reddish tinge, potentially indicating the presence of older, redder stars. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers, though subtle disturbances in the outer halo cannot be ruled out without higher resolution imaging. The overall shape is slightly elongated, but generally consistent with an elliptical morphology. The galaxy appears relatively inactive in terms of star formation, given the smooth structure.
