The galaxy presents as a generally smooth, centrally concentrated object with a high degree of circular symmetry. There is no obvious presence of spiral arms, bars, or distinct disk-like features. The color profile suggests a relatively old stellar population, with a dominant reddish hue in the central region that transitions to a slightly more greenish-yellowish tint toward the outer edges. The overall appearance is consistent with an elliptical galaxy or potentially a lenticular galaxy viewed face-on. There may be some indication of minor tidal disturbances or interactions, but the overall structure remains largely undisturbed.
