The galaxy exhibits a generally elliptical morphology with a high degree of smoothness in its light distribution. There's a pronounced central bulge that dominates the overall luminosity, appearing as a concentrated and bright region. Fainter, more diffuse light extends outwards from the bulge, forming a halo that appears flattened. The overall color profile suggests a relatively evolved stellar population. There is likely very little or no ongoing star formation. There is a very slight presence of a disk. There are no obvious signs of strong tidal disturbances or recent mergers in the image.
