The galaxy presents a largely smooth morphology, appearing elliptical in shape, with a high degree of central concentration. Its core exhibits a bright, yellowish-orange color, suggesting an older stellar population. The galaxy's halo displays a gradual decline in surface brightness away from the center. The galaxy's outer regions show a mottled texture indicative of a combination of older stars and dust. Subtle hints of a weak, disturbed disk-like structure may be present around the core, however, this is not significant. Overall, the galaxy appears to be relatively isolated and quiescent.
