The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology with a slight elongation. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions possess a subtle bluer tint, hinting at the presence of some younger, hotter stars, although the overall color suggests that the galaxy is relatively evolved. There are subtle indications of some minor disturbances, with potential faint tidal features extending from the main body. There are no definitive signs of a major merger in progress. The object appears predominantly spheroid in shape, with a moderate degree of ellipticity.
