The galaxy presents as a smooth, elliptical morphology. It exhibits a pronounced central bulge that transitions smoothly into the outer regions. The color gradient suggests a population of older stars dominating the central region, indicated by the yellowish hue, with bluer tones appearing in the outer regions, potentially indicative of some younger stellar populations or ongoing, albeit limited, star formation. There is no visible evidence of spiral arms, significant dust lanes, or major disturbances suggestive of recent major merger activity, although a slight irregularity could point to a minor interaction in the past. The overall shape is elongated, with a cigar-like appearance.
