The object presents as a single galaxy with a relatively smooth morphology. The galaxy displays a slight elongation, deviating somewhat from a perfectly circular profile. There is a color gradient, shifting from a yellowish center to a bluer color in the periphery, suggesting a difference in stellar population, with the center containing older stars and outer regions exhibiting younger stellar populations. Overall, the galaxy appears relatively undisturbed, showing no major signs of active merging or tidal disruptions. There are likely some disk or spiral features present, though they are not completely distinct. Based on the observed color distribution, the galaxy is likely undergoing a low level of star formation.
