The galaxy appears to be a spiral type, observed at a moderate inclination. Two prominent spiral arms are discernible, exhibiting a loose winding pattern. The central bulge is of moderate size, with a somewhat elongated shape, and exhibits a yellow-white hue, indicating an older stellar population. The arms display patches of blue, suggestive of ongoing star formation within them, but the color is most likely dominated by older stars. There is no obvious bar structure. The galaxy's disk is not perfectly smooth; there are some irregularities, but it appears to not be undergoing any major mergers.
