The galaxy presents as a somewhat smooth, elliptical-like structure. It exhibits a concentrated core region with a centrally peaked brightness profile, indicating a significant bulge component. The galaxy appears to have a slight elongation, but is mostly round in appearance, with some degree of tidal disturbance. The color index suggests it may be composed of aging stellar populations. A region appears to be forming a faint tail. No prominent spiral arms or dust lanes are discernible within the current image resolution.
