The galaxy appears to be a somewhat rounded system, exhibiting a relatively smooth morphology. There is a degree of interaction apparent, characterized by what seems to be a smaller merging component in the system. The dominant body shows a color gradient, transitioning from a bluer hue in its outer regions to a yellower core. The bluer color suggests ongoing star formation within the disk, while the yellowish color of the central bulge suggests the presence of an older stellar population. The galaxy has a noticeable degree of internal structure, hinting at the potential presence of spiral arms or other disk-like features, though these features are not sharply defined. Overall, the galaxy seems to be in an intermediate stage of its evolution, undergoing active star formation but also displaying characteristics of a more evolved system.
