The galaxy presents a generally smooth, elliptical morphology. Its core region exhibits a bright, concentrated luminosity, transitioning outwards to a more diffuse halo. The overall color profile leans towards the redder end of the spectrum. There is very little evidence of spiral arm structure. A slight asymmetry can be noted in the galaxy's outer regions, possibly indicative of minor tidal interactions, although major disturbances are not apparent. There is a small, slightly bluer region that could be the result of localized star formation.
