The galaxy presents a predominantly elliptical morphology, though with hints of a disk-like structure. A central bulge dominates the light profile, exhibiting a reddish hue, suggesting an older stellar population. The outer regions show a bluer color, which may indicate more recent star formation activity, but the fraction of blue light is small. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal features. There might be some minor perturbations in the disk, potentially indicating minor disturbances. The galaxy’s smooth appearance is moderately pronounced, but not completely spheroidal.
