The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge with decreasing surface brightness moving outward. The core exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions display a bluer tint, indicative of the presence of younger, hotter stars. The overall shape is mostly round, with minimal deviation from a spherical form. Faint, diffuse extensions are barely perceptible, possibly indicating tidal interactions or minor disturbances. There are no apparent dust lanes or prominent spiral arm structures visible, however, the faint blue tinge in the outer regions suggests possible, yet faint, star formation.
