The galaxy presents a generally smooth morphology, with an apparent spheroidal shape. The light distribution is centrally concentrated, appearing brightest in the core region. There is a gradual decrease in luminosity moving outward from the center. The galaxy exhibits a reddish-yellow hue, potentially indicating a population of older stars and a relatively low rate of ongoing star formation. There is minimal evidence of spiral arm structure or significant dust lanes, and there are no apparent major disturbances or merging features. Overall, the galaxy seems to be relatively undisturbed and relaxed, with a somewhat elliptical form.
