The galaxy presents as an elliptical morphology, with a smooth and centrally concentrated light distribution. The color gradient suggests the presence of an older stellar population concentrated in the core, appearing reddish-yellow, with a transition to a bluer population in the surrounding regions. There is no evidence of spiral arms, dust lanes, or significant star-forming regions. The overall appearance indicates a relatively evolved galaxy, potentially with ongoing, but low-level star formation. The galaxy appears undisturbed, with no signs of significant tidal interactions or recent mergers. The ellipticity suggests a moderate degree of rotational support.
