The galaxy presents as a roughly elliptical, centrally concentrated object. The core exhibits a bright, yellowish-white luminosity, suggesting a substantial population of older stars. Moving outward from the core, the intensity gradually decreases, forming a smooth, diffuse halo. Some slight asymmetry is apparent in the outer regions, hinting at potential tidal interactions or past minor disturbances, though a well-defined spiral structure is not discernible. There is some slight bluer coloration near the extremities, possibly indicative of some ongoing star formation. The overall color profile suggests a galaxy dominated by an older stellar population, with relatively low levels of current star formation activity.
