The galaxy presents as a centrally concentrated, elliptical-like structure. The core is a bright, yellowish-white, suggestive of an older stellar population. Moving outwards from the core, the galaxy exhibits a gradual decrease in luminosity, transitioning to a blueish, less intense halo. There is no apparent spiral arm structure or significant dust lane obscuration visible in the image. The galaxy's overall shape appears moderately elongated. There is no evidence of a major ongoing merger event. The system displays a smooth profile, indicative of a lack of significant recent star formation and disturbances.
