The galaxy appears to be a spiral galaxy viewed at an oblique angle, suggesting a disk-like structure. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population. The disk component surrounding the bulge shows a slightly bluer coloration, suggestive of ongoing star formation. The spiral arms are not sharply defined, lending a somewhat flocculent appearance to the galaxy. Overall, the galaxy presents a moderately smooth morphology, but the presence of some irregularity and subtle color variations within the disk may indicate past or ongoing interactions or internal dynamical processes. It seems to have an intermediate roundness, between round and cigar-shaped. There is no evidence of a major merger.