The galaxy presents an overall smooth morphology. It exhibits a concentrated central bulge, characterized by a yellowish-white hue, indicating a population of older stars. A somewhat diffuse halo surrounds the central bulge, which is less luminous and has a slightly bluer tint, possibly suggesting the presence of younger stellar populations or ongoing star formation. The galaxy displays a moderately elliptical shape, with no prominent spiral arm structures visible. There appears to be minimal evidence of tidal disturbances or ongoing mergers. The system is well-defined but not perfectly circular.
