The galaxy appears to be an interacting system, possibly in the early stages of a merger. There are two primary components: a bluer, less concentrated region to the left and a yellower, more concentrated region to the right. The bluer component shows evidence of ongoing star formation. It has a relatively smooth appearance with a diffuse structure, hinting at a possible disk-like morphology. The yellower component exhibits a more concentrated, elliptical-like morphology. It shows a smoother distribution of light, suggesting an older stellar population with less recent star formation. There is a faint bridge of material appearing to connect the two components. Overall, the galaxy is relatively compact. It displays hints of tidal features or disturbances suggesting a possible merger.
