The galaxy presents as a moderately inclined disk galaxy. It exhibits a bright, concentrated central bulge, which appears yellowish-white, suggesting a population of older stars. The disk is relatively smooth in appearance and exhibits a bluer hue than the bulge, possibly indicative of ongoing star formation. There is subtle evidence of spiral arm structure, though it appears tightly wound and less distinct. The galaxy appears elongated, with the major axis oriented roughly horizontally. The outer regions of the disk fade gradually into the background, indicating a lack of a sharp cutoff. The overall morphology suggests a relatively evolved spiral galaxy.
