The galaxy appears as a moderately inclined, elongated spiral. There is evidence of a disk-like structure, although the spiral arms are not sharply defined, but appear more flocculent. The central bulge seems small compared to the overall size of the disk. The color gradient indicates a possible presence of older stellar populations in the central regions, appearing more yellow/orange, while the outer regions of the disk exhibit a bluer hue, suggesting ongoing star formation. There are no obvious signs of major mergers or tidal disturbances in this image. A slight asymmetry may indicate a minor interaction, but overall, the galaxy appears relatively undisturbed.
