The galaxy presents as a generally elliptical morphology, though with some irregularities. The core is relatively bright, with a diffuse, somewhat mottled halo extending outwards. There may be the beginning signs of a disk, however it appears somewhat disturbed. There is some indication of blue star formation regions, primarily in the "disk" sections, suggesting ongoing, though potentially declining, star formation. The galaxy appears to be relatively isolated. A visual inspection suggests it is of intermediate mass. The halo exhibits no immediately apparent tidal features suggesting past recent mergers or disturbances. It is difficult to asses if a supermassive black hole exists in the galactic center, but, based on the color and star formation rate, it is likely.
