The galaxy presents a clear spiral structure. Two prominent spiral arms emanate from a central, relatively bright bulge. The arms are fairly well-defined, displaying a moderate winding pattern as they extend outwards. The arm structure appears relatively symmetric. The central bulge exhibits a yellowish hue, possibly indicating a population of older stars. Patches of blue are visible within the spiral arms, suggesting regions of active star formation. There is a slight indication of a bar-like structure. Overall, the galaxy exhibits a normal spiral morphology with no obvious signs of major interactions or significant distortions. It appears to be a relatively isolated and well-formed system.