The galaxy appears to be a relatively smooth, elliptical system. It presents a concentrated central bulge, with the luminosity appearing to gradually fade toward the outer edges. The overall shape is moderately elliptical; it is not perfectly spherical, but also not highly elongated. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests a population of older stars, with a yellowish-red hue dominating the galaxy's overall light output. The absence of obvious blue regions implies a low rate of on-going star formation. There is no clear indication of a major ongoing merger event, though some slight irregularity in the outskirts might point to a minor interaction in the past. The estimated size suggests that this galaxy is likely a large system.
