The galaxy presents as a slightly elongated spheroid with a smooth, diffuse appearance. It exhibits a concentrated central bulge that is characterized by a yellowish-orange hue, suggesting a population of older, evolved stars. The outer regions of the galaxy appear fainter and somewhat redder, potentially indicating a lower density of stars or the presence of dust absorption. There are hints of a very faint disk, but no clear spiral arm structure or prominent features are visible. The overall morphology indicates a lack of ongoing major star formation. There are no obvious signs of recent mergers or significant tidal disturbances. The general smoothness and color profile are consistent with an elliptical galaxy or a lenticular galaxy viewed at an angle.
