The galaxy presents as a spiral type, seen face-on. It exhibits a distinct central bulge that appears small relative to the overall disk size. Spiral arms are prominent and well-defined, displaying a tightly wound morphology. Evidence suggests the presence of at least two and perhaps three spiral arms. A weak bar structure appears to be present, extending through the central region of the bulge. There does not appear to be any major merging occurring, however, there does appear to be some minor disturbances in the disk. The disk appears to dominate the overall morphology, with minimal evidence of a large or dominant bulge.
