The galaxy presents a relatively smooth, elliptical morphology. Its color profile appears somewhat red, concentrated towards the center, suggesting a population of older stars and a possible dearth of active star formation. The galaxy displays a slight elongation and lacks any apparent spiral arm structure or significant dust lanes. There is no evidence of a recent major merger or tidal disturbances. The core is noticeably bright, indicating a possible active galactic nucleus. The galaxy is relatively compact.
