This galaxy presents as a relatively smooth, elliptical or lenticular system. The central bulge is prominent and exhibits a concentrated, bright luminosity. The overall shape is predominantly round. There is a faint, diffuse halo surrounding the brighter core, showing a gradual decrease in luminosity outwards. There appears to be minimal to no evidence of spiral arm structure or significant dust lanes. The galaxy's color profile suggests a population dominated by older stars. There is a subtle blueish hue within the outer regions, possibly indicating a small amount of on-going star formation. Overall, the galaxy appears as an isolated system with no immediately obvious signs of major mergers or tidal disturbances.
