This galaxy presents as a relatively smooth object with a largely elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes, suggesting it is primarily composed of older stellar populations. The light is fairly uniform across the galaxy, with a slight central brightening. Overall, the galaxy appears to be relatively isolated, showing no signs of major disturbances or ongoing merger activity. Its color is moderately red, indicative of a more evolved system with reduced star formation.
