The galaxy appears as a slightly elongated spheroid, possibly an elliptical galaxy, with a smooth, concentrated light profile. Its core exhibits a yellowish hue, indicating a population of older stars. There's a gradual decrease in luminosity moving outward from the center, with a faint, diffuse halo of bluish light surrounding the core, perhaps a contribution from a younger stellar population. The overall structure shows little evidence of spiral arms or significant dust lanes, suggesting a lack of active star formation. There appears to be no signs of any tidal disturbances or ongoing mergers.
