The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. The overall shape appears largely rounded, with a minimal deviation from circular symmetry. There is no clear evidence of prominent spiral arms or a well-defined disk structure. Faint color variations are visible across the galaxy's body, suggesting possible differences in stellar populations or dust distribution. No significant signs of ongoing major mergers or tidal disturbances are apparent. The galaxy appears to be relatively isolated within the observed field.
