The galaxy appears to be a relatively small, disk-shaped system seen at a moderately inclined angle. The central bulge region is bright and concentrated, with an off-white to yellow-white hue, suggesting an older stellar population. Extending outward from the core is a bluish-green disk that surrounds the bright central region. The bluish coloration hints at the presence of ongoing star formation within the disk. The disk itself appears somewhat irregular and clumpy, suggesting potential interactions or internal disturbances. The overall impression is of a system that may be undergoing some evolutionary change, although it mostly appears smooth. There is no immediately discernible evidence of any major merging events based on the image.
