The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The overall color is yellowish-orange, suggesting a population of older stars. The galaxy does not appear to exhibit any distinct spiral arm structure or signs of recent major merger events. It is slightly elongated in shape, being somewhere between round and cigar shaped. There is some evidence of a faint halo extending beyond the main body of the galaxy, though the outer edges are somewhat indistinct. Based on the data, there may be only minor disturbances, if any, and a low star formation rate.
