The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright central bulge that appears nearly spherical and dominates the overall luminosity profile. Moving outward from the core, there is a gradual decrease in surface brightness. The outer regions show a faint disk-like structure, however it is not clearly resolved into spiral arms or distinct features. There may be some degree of internal dust obscuration, but it does not appear significant in the overall structure. The galaxy exhibits a subtle color gradient, with the core appearing yellower and the outer regions showing hints of bluer colors. This suggests some presence of younger stellar populations in the outer regions. There is no apparent evidence of significant recent mergers or tidal disturbances. The shape indicates the galaxy is likely an intermediate type between elliptical and spiral, possibly an S0 or early-type spiral.
