The object appears to be a spiral galaxy at a considerable distance. It exhibits a prominent disk structure with a discernible central bulge. The spiral arms are visible, albeit somewhat flocculent, suggesting a moderate degree of ongoing star formation. The galaxy appears to be undergoing some form of interaction, given the disturbed morphology. There is a suggestion of tidal features or merging activity; the disk is not perfectly symmetric, and there may be a companion galaxy contributing to the observed disturbance. The bulge appears yellowish, indicating an older stellar population, while bluer regions within the disk suggest areas of recent or active star formation. The galaxy's orientation is close to face-on, allowing for a relatively clear view of its spiral structure. The galaxy has some bar structure. The size of the galaxy is moderate.
