This galaxy presents as a relatively smooth, elliptical-like structure. It appears to be largely featureless, lacking prominent spiral arms or a well-defined disk. The light is concentrated towards the center, creating a bright, well-defined core.

The color profile is slightly redder in the core and slightly bluer in the outer halo, indicating that the population of stars is older in the core than the outer halo. It exhibits a generally symmetrical shape, without any obvious signs of major tidal disturbances or ongoing mergers. There might be subtle asymmetry hinting at a minor interaction, but the overall morphology is consistent with a relaxed system. The lack of a clear disk suggests that it is a relatively old and dynamically settled system, where star formation rates are currently low, with older stars concentrated in the core of the galaxy. The lack of visible dust lanes supports this conclusion.
