The galaxy presents as a single, somewhat elongated object, exhibiting a smooth light profile across its visible extent. The central region is significantly brighter and slightly bluer, suggesting a concentration of younger, hotter stars or possible active galactic nucleus activity. The outer regions appear redder, potentially indicating an older stellar population or dust absorption. The overall shape is not perfectly circular, showing a degree of elongation, possibly indicative of an elliptical morphology or a disk seen at an angle. No distinct spiral arms or bars are discernible. There is a potential tidal tail or faint, distorted feature extending outwards. This galaxy exhibits characteristics that place it in the transition region between elliptical and lenticular galaxies.
