The galaxy presents a flattened, disk-like morphology. There is an indication of spiral arm structure, appearing somewhat disturbed or flocculent, rather than well-defined. The central bulge is prominent and exhibits a yellow-white hue, suggestive of an older stellar population. The outer regions of the disk show bluer colors, potentially indicative of more recent star formation. The overall form appears slightly elongated, though without a pronounced cigar-like shape. There is a suggestion of interaction or tidal disruption in the surrounding area, but the main galaxy body is largely intact. Although generally smooth in appearance, there is a presence of some features in the galaxy, rather than it being completely uniform.
