The galaxy appears as a somewhat diffuse, centrally concentrated object. It presents a fairly smooth profile with a hint of a flattened disk-like structure oriented roughly horizontally. A subtle color gradient is observable, with a bluish tint towards one side and a gradually redder hue towards the other. The object's light distribution implies a dominant stellar population likely composed of both young stars and older redder stars, suggesting ongoing star formation. There is some indication of interaction with a nearby galaxy in the form of faint tidal features, though this requires further investigation. The central region appears slightly brighter and more concentrated, potentially indicating the presence of an actively star-forming core or possibly a supermassive black hole. A low level of dust extinction could be present.
