The galaxy exhibits a relatively smooth morphology, with a dominant spheroidal component. Its shape appears to be transitioning between round and elliptical. There are hints of a disk structure, although it is not prominent. The central region is bright, suggesting a concentration of stars or possibly an active galactic nucleus. The color profile indicates varying stellar populations; the core shows a greater intensity of red, potentially due to older stars, while a dimmer region has a stronger blue component, suggestive of younger stars. Overall, the galaxy appears relatively undisturbed, with no significant signs of tidal interactions or major mergers. It's moderately large, with indications of ongoing star formation at a low to moderate rate.
