The galaxy presents as a relatively compact and smooth object. It exhibits a roughly elliptical morphology, appearing largely undisturbed with no obvious tidal features or signs of major mergers. The light distribution is concentrated towards the center, suggesting a significant bulge component. A subtle color gradient is noticeable, with the central regions appearing slightly redder compared to the outer regions, potentially indicating an older stellar population in the core. There are possible hints of a faint, extended halo, but the signal is weak.
