The galaxy presents as a roughly elliptical, concentrated light source, generally smooth in appearance. The color profile appears to be relatively uniform across the galaxy, trending slightly towards the redder portion of the spectrum. There is no visually discernible spiral structure or pronounced dust lane obscuration. A fainter, less defined light concentration can be observed nearby, with the suggestion of a tidal interaction. There are no large-scale disturbances evident in the main body of the galaxy. This galaxy likely harbors a large mass of stars, with a low rate of star formation. It is likely classified as a late-stage galaxy which has seen most of its star formation conclude.
