The galaxy presents as a primarily smooth object with an elliptical morphology. Its overall shape approximates a somewhat elongated spheroid, appearing more "in between" round and cigar-shaped. The central region displays a concentrated luminosity, exhibiting a yellowish-white hue, suggestive of an older stellar population and minimal recent star formation activity. Fainter, blue-tinged regions are visible on the outer edges of the galaxy, indicating the presence of at least some younger stars. There is no obvious evidence of spiral arm structure or a distinct disk component, but a slight asymmetry in the distribution of light within the fainter regions might suggest the presence of a minor disturbance. Overall, the galaxy appears relatively isolated, showing no strong signs of a major ongoing merger, though there might be a sign of minor disturbance on the outer edges. The galaxy has an apparent magnitude of around 18.