The galaxy presents an elliptical morphology, with an apparent disk component. The central bulge exhibits a bright, concentrated luminosity profile, suggesting a significant population of older stars. A faint, diffuse halo surrounds the central region, extending further along the major axis than the minor axis. The light distribution appears relatively smooth, with only subtle variations in color and intensity. Subtle indications of a possible dust lane are seen along the major axis. The overall color is generally redder, indicative of an older stellar population. The galaxy appears relatively isolated, showing no signs of recent major mergers or tidal interactions.
