The galaxy presents a largely smooth, elliptical morphology. Its light profile is concentrated toward the center, exhibiting a bright, yellowish core that diminishes gradually outward. The overall shape appears to be somewhere between round and oblong, with no obvious spiral arm structure or pronounced disk component. The galaxy exhibits a distinct color gradient; the central region appears yellower, possibly indicating an older stellar population or dust obscuration. The light distribution is mostly uniform, with no strong evidence of ongoing mergers or major disturbances. Minor irregularities are possible, but are not clear due to image resolution. The galaxy's red color suggests a relatively low star formation rate. The overall impression is that of a relatively quiescent, evolved system.
