The galaxy exhibits a centrally concentrated, smooth morphology, with an elliptical shape. The core region displays a bright, yellowish-white color, indicative of an older stellar population. A gradual decrease in surface brightness is observed moving outward from the core, with the color transitioning to a slightly redder hue in the outer regions, suggestive of a mix of stellar ages, with older stars dominating. There appears to be minimal evidence of distinct spiral arm structures or significant dust lanes. There is a slight asymmetry visible in the lower left quadrant, which could be due to a minor tidal interaction or internal structure.
