The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellow-white hue, suggesting a population of older stars. The luminosity appears to decrease gradually from the core outwards, forming a diffuse halo. There is little to no evidence of spiral arms or significant dust lanes within the visible spectrum. The overall shape is predominantly round, with a slight deviation towards a more oblong form. There are hints of minor disturbances or asymmetry in the outer regions, but no signs of a major ongoing merger or significant tidal disruption. The colour profile suggests a lack of substantial recent star formation.
