The galaxy presents as a centrally concentrated object with a smooth overall morphology. The central region displays a bright, yellowish-white core, suggesting a significant population of older stars. The light gradually diffuses outward from the core, transitioning to a less concentrated halo. Subtle color variations are observable in the halo, with faint reddish hues indicating areas of potential older stellar populations or dust obscuration. The galaxy exhibits a roughly elliptical shape but also seems to be undergoing some gravitational disturbance, with a slight asymmetry in the halo. Possible faint tidal features or merging activity are present but difficult to fully resolve due to the image's resolution. The color profile indicates ongoing but moderate star formation, with the bulk of its stellar mass likely composed of an older population.
