The observed galaxy appears as a relatively compact object. Its light is dominated by a central, bright, and somewhat diffuse core. This core exhibits a bluish-white hue, indicating the presence of hotter, younger stellar populations. The overall morphology suggests that the galaxy is primarily smooth in appearance. There is no obvious spiral arm structure or dust lane features visible in the image. There are some signs of possible interactions from other objects nearby that appear to affect the shape of the galaxy. Overall, the system seems to be fairly circular, with a minor extension to one side.
