The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, diminishing outward. The object appears to be moderately bright in this observation. There is a suggestion of a slight color gradient from the core to the outer regions, with the core appearing somewhat bluer and outer regions appearing redder, although this may be slight. No prominent spiral arms or significant dust lanes are discernible. There is no obvious tidal distortion or interaction with nearby galaxies. The galaxy presents as non-merging, without indications of major or minor disturbances to its overall structure.
