The galaxy presents a smooth, elliptical morphology. It is characterized by a bright, concentrated central bulge which transitions gradually into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish hue dominating the central regions, indicative of evolved stars. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer, potentially indicating a small amount of ongoing star formation, although this is not immediately obvious. There are hints of a possible minor disturbance in the structure. It does not appear to be actively merging with any other large galaxy, though it is possible that there are minor tidal features present, but not readily apparent in the data.
