The galaxy presents a generally smooth, elliptical morphology with a notable central bulge. The light distribution appears concentrated towards the center, with a gradual decrease in intensity moving outward. There is a slight elongation in the galaxy's shape, deviating minimally from a perfectly circular form. Color gradients are subtle, with a tendency towards redder hues in the central region, possibly indicating an older stellar population. Fainter, bluer regions exist in the outer parts of the galaxy, suggesting the presence of younger stars or regions of recent, though minimal, star formation. There are no readily apparent signs of strong tidal interactions or major disturbances in its structure. The overall appearance suggests a relatively evolved system, with a dominant smooth component and only subtle features indicative of ongoing activity.
