This appears to be a spiral galaxy, observed at a relatively face-on orientation. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. Fainter spiral arms extend outwards from the central bulge. The arms show some irregularity in their structure, with a winding that could be considered intermediate between tight and loose. The galaxy exhibits a relatively high degree of symmetry in the overall spiral structure, with two dominant spiral arms. There is also an indication of a bar-like structure in the central region of the galaxy. There is no obvious visual evidence of a major merger event, although subtle disturbances may be present. The galaxy does not appear to be perfectly smooth; in fact, it shows a reasonable number of features, including the disk and spiral arms. The color gradient suggests ongoing star formation within the disk.