The galaxy presents as a generally smooth, round, and somewhat compact object. There is a central concentration of light that appears yellowish-orange, possibly indicating an older stellar population and/or significant dust obscuration. The outer regions appear slightly greener in hue, potentially suggesting a minor amount of ongoing star formation, but the overall lack of distinct spiral arms or other features indicates a relatively passive system. There is no visible evidence of a major merger or significant tidal disturbance, and the galaxy appears relatively isolated and undisturbed. The overall morphology is consistent with that of an elliptical galaxy.
