The galaxy presents a generally smooth morphology with a central concentration of light, suggesting a prominent bulge. The overall shape is elliptical, though it deviates slightly from being perfectly round. The color gradient indicates a redder core transitioning to a bluer, more diffuse halo or outer region. There is no obvious spiral arm structure or significant dust lane obscuration. The object does not appear to be undergoing a major merging event, though there might be some minor distortions in the outer isophotes, possibly indicative of a minor interaction or past merger. The galaxy's low rate of star formation may contribute to the lack of bright, blue star-forming regions.
