The galaxy appears as a largely featureless, elliptical-like structure with a concentrated, bright central bulge. The core exhibits a reddish-orange hue, suggestive of an older stellar population and a lack of significant recent star formation activity. Fainter greenish-yellow emissions surround the bright bulge, possibly indicating some presence of younger stars or ionized gas, although these features are not prominent. The overall morphology is smooth and rounded, lacking any signs of spiral arms or significant dust lanes. There is no readily apparent indication of tidal disturbances or ongoing mergers.
