The galaxy appears to be a relatively compact, elliptical system. Its light profile is smooth, with a concentrated central region. The galaxy exhibits a yellow-red color, indicative of an older stellar population and potentially, a lack of significant ongoing star formation. There is no discernible disk structure or spiral arm morphology. The overall form is generally round, lacking any significant elongation. There is no obvious evidence of major mergers or tidal disturbances in its immediate vicinity. The object is likely a massive galaxy, given its brightness and inferred distance.
