This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears bright and yellowish, possibly indicating an older stellar population. The light fades gradually moving outward from the core to the edge, with a more diffuse, blue-ish halo surrounding the central region. There is little evidence of spiral arm structures or significant dust lanes. No obvious signs of tidal disturbances or ongoing major mergers are visible in the image. The galaxy appears fairly isolated, without any companion galaxies nearby that could be interacting. Overall, it seems to be a well-formed galaxy.
