The galaxy presents as a smooth, centrally concentrated elliptical. The light distribution indicates a generally spheroidal morphology, with a bright, relatively compact core that likely hosts a supermassive black hole. There is little evidence of spiral arms or a disk-like structure. There is a slight elongation with the major axis running roughly horizontal in this orientation, but it is mostly round. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a bluish periphery, suggesting a change in stellar populations with radius. The redder colors in the core indicate older stars, whereas the bluer colors in the outskirts could indicate more active star formation in these regions, or a population of younger, bluer stars. The galaxy appears relatively isolated, without strong signs of tidal interactions or ongoing mergers. There may be minor disturbances, but they do not appear to have significant impact. Overall, it appears to be a relatively relaxed, evolved system.
