The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth luminosity profile. The light distribution appears relatively even with no prominent spiral arm features or distinct substructures discernible. It has an overall round morphology with only minor deviations from a perfect circle. A slight elongation along one axis is possibly visible. The galaxy exhibits a color gradient, appearing more yellowish-red towards its core, suggesting a higher concentration of older stellar populations in the central region. The outer regions have a bluer tint, hinting at younger stars. There is no obvious indication of ongoing major mergers or tidal disturbances affecting the galaxy's overall shape, although there is potential for minor disturbances. The smooth, featureless nature of the galaxy is consistent with a relatively passive system where star formation is suppressed.
