The galaxy appears to be an elliptical type, with a generally smooth morphology. It displays a concentrated central bulge, exhibiting a yellowish-orange hue, indicative of an older stellar population. The outer regions show a faint, diffuse halo with slightly bluer tones, suggesting the presence of some younger stars, but the overall color indicates that star formation activity is relatively low. The galaxy exhibits a notable degree of roundness, with no discernible spiral arm structure or strong tidal features, and there is no indication of a major ongoing merger. Minor disturbances cannot be ruled out.
