The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. There is a lack of discernible spiral arm structure or dust lanes. The overall color is yellowish-orange, which suggests an older stellar population with fewer young, hot stars. The light is centrally concentrated, with luminosity appearing to decline gradually towards the edges of the galaxy. The galaxy appears isolated, with no visually obvious signs of recent or ongoing major mergers. There is possibly a faint tidal tail or minor disturbance on one side, suggesting a potential minor interaction in the past. The galaxy has a round morphology, with no signs of being cigar-shaped.
