The galaxy presents a relatively smooth, elliptical morphology. It appears largely featureless with a centrally concentrated luminosity profile. The galaxy exhibits a yellowish-white hue, potentially indicative of an older stellar population. Its overall round shape suggests little to no rotational support. There are no apparent signs of ongoing mergers or major disturbances; it seems to be a fairly relaxed system. The color distribution is relatively uniform across the galaxy, suggesting a lack of significant dust lanes or prominent star-forming regions.
