The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge that decreases in luminosity at the edges. It is generally round in shape. There is no clear sign of spiral arm structures, a prominent disk, or any obvious ongoing major merging events. The galaxy appears to be relatively isolated, with no nearby companion galaxies that would indicate a strong interaction. Overall, the galaxy appears to be a mature system, potentially an early-type galaxy, with no indication of active star formation. Its red-yellow hue suggests an older stellar population. There are slight hints of disturbed features, potentially indicating minor past interactions, but overall the galaxy is well-formed.
