The galaxy appears to be a relatively smooth, lenticular type, exhibiting an elliptical morphology. Its luminosity profile suggests a centrally concentrated bulge with a gradual decrease in surface brightness towards the outer regions. Color gradients are visible, with the central region appearing more yellow-red, indicating an older stellar population and/or dust obscuration. The outer regions appear slightly bluer, hinting at the presence of younger stars or less dust. The galaxy doesn't show any prominent spiral arm structures or significant signs of recent mergers or major disturbances, although there are some irregularities within the light distribution of the galaxy, indicating there may be a minor disturbance. It's axial ratio suggests an "in between" shape, meaning it does not appear to be too rounded or too cigar-shaped. Overall, the galaxy appears as a matured system, undergoing passive evolution.
