The galaxy exhibits a primarily smooth morphology, with some features that suggest a disk-like structure. It displays a shape that is neither perfectly round nor highly elongated, falling into an intermediate category. There is a notable central bulge, which appears yellowish, suggesting an older stellar population. The outer regions are bluer in color, potentially indicating regions of recent star formation, and the overall structure suggests the possibility of a spiral galaxy, seen at some angle. There are no obvious signs of ongoing major merger activity, although minor disturbances might be present.
