This galaxy appears to be a spiral galaxy observed at an angle between face-on and edge-on. There is a noticeable central bulge that exhibits a yellowish hue, suggesting an older stellar population. The spiral arms are somewhat diffuse and appear blueish, potentially indicating ongoing star formation. The dust lanes in the spiral arms are not clearly defined. There appears to be some minor disturbance within the disk structure. The overall form does not show any evidence of major mergers, though the spiral arms have non-uniform densities. The size of the central bulge, relative to the disc, suggests a relatively massive galaxy.
