The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a centrally concentrated luminosity profile with a bright, yellowish core, indicative of an older stellar population. The outer regions show a gradual decline in brightness, with a subtle bluish tinge, potentially suggesting the presence of younger stars in the outskirts, or a slightly bluer population. The galaxy's overall shape is somewhat elongated, appearing more rounded than highly flattened. There is no strong evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears to be an evolved system with a dominant bulge component.
