The galaxy exhibits a prominent disk structure. It presents a spiral morphology, with two distinct, well-defined spiral arms emanating from the central bulge. The winding of these arms appears to be of medium tightness. A bar-like feature is visible, extending across a significant portion of the galaxy's central region, showing evidence of both a strong and weak feature. The galaxy's bulge is moderately sized relative to the disk. There are no indications of major ongoing merger activity, although there may be minor distortions in the disk, suggesting a possible recent interaction or disturbance. The overall color gradient of the galaxy indicates a population of both older stars in the central bulge, with indications of star formation occuring in the spiral arms. The galaxy is not observed edge-on.