The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile. The light distribution is relatively smooth, with minimal discernible substructure, spiral arms, or dust lanes. Color gradients are subtle. The core exhibits a yellow-white hue, which transitions to a bluer tint towards the outer regions. The overall appearance suggests a gravitationally relaxed system, likely dominated by an older stellar population with ongoing, but limited, star formation. There is no visual evidence of a major merger or significant tidal disturbances, indicating a stable evolutionary state.
