The galaxy appears to be elliptical in shape with a smooth, diffuse light distribution. The core is bright and concentrated, exhibiting a yellow-orange hue, suggestive of an older stellar population. Progressing outwards from the center, the galaxy gradually fades into a fainter, blueish halo. This color gradient implies the presence of some ongoing, but low-level, star formation in the outer regions, or perhaps a population of younger stars. There is no visible evidence of spiral arms or a distinct disk structure. The galaxy seems relatively undisturbed, lacking obvious signs of tidal interactions or major mergers, with perhaps a very minor asymmetry hinting at a previous interaction.
