The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color is yellowish-white, suggesting a population of older stars. There's a subtle elongation, but the galaxy is mostly rounded. No distinct spiral arms or prominent dust lanes are visible, indicating a lack of significant ongoing star formation within a well-defined disk structure. The outer regions of the galaxy gradually fade into the background, lacking sharp boundaries or tidal features indicative of recent major interactions. There is some evidence of minor disturbances.
