The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a bright, somewhat diffuse core. There's a subtle color gradient visible, trending from a yellowish central region to a slightly redder outer halo, suggesting potential differences in stellar populations or dust content between the core and the outer regions. The overall morphology appears undisturbed; no clear signs of tidal features, strong asymmetries, or ongoing major merging events are immediately apparent. The galaxy's general roundness suggests a minimal degree of rotational support. There is limited evidence of ongoing star formation.
