The galaxy appears as a relatively smooth, centrally concentrated object with a nearly circular morphology. There is a bright central region that likely represents the core of the galaxy. The light appears to gradually fade outward from the core, with no obvious spiral arm structures or distinct features visible at this resolution. The overall color is consistent with an older stellar population. There is a subtle color gradient, with the central region appearing slightly bluer compared to the outer regions. The galaxy exhibits a relatively uniform structure, with no clear signs of significant disturbances or interactions.
