The galaxy appears as a fairly smooth, elliptical-like structure with a high degree of central concentration. It is nearly circular in projection. There is little evidence of spiral arm structure, disk-like features, or significant tidal disturbances from interactions with other galaxies. The galaxy exhibits a color profile that is relatively uniform across its extent, suggesting a fairly homogenous stellar population. The overall color index indicates the presence of older stars. There is limited evidence of on-going star formation, which is consistent with its morphology. The mass estimate indicates a fairly massive galaxy, likely within the range of an average elliptical galaxy.
