The galaxy presents as a centrally concentrated, elliptical-like structure, with a smooth, featureless appearance. The color gradient suggests a concentration of older stellar populations towards the core, indicated by a yellowish hue. The outer regions appear fainter and exhibit a subtle blue tinge, implying the presence of younger stars, but to a significantly lesser extent compared to the central bulge. There is no obvious spiral arm structure or significant dust lane visible. The overall shape appears nearly round with only a hint of elongation. There are no indications of any major ongoing mergers or tidal disturbances. The galaxy is compact in size and exhibits a fairly symmetrical morphology.
