The galaxy presents a notable disk-like structure with evidence of spiral arms. The arms appear somewhat fragmented and not uniformly distributed, suggesting potential gravitational interactions or internal disturbances. The spiral arms have a medium winding. The galaxy exhibits a prominent central bulge, which is estimated to be of moderate size compared to the disk. It appears relatively luminous, possibly indicating a high concentration of older stars and a supermassive black hole at the galactic center. The colors within the galaxy vary, with the central bulge appearing more yellow, indicating older stellar populations, while the spiral arms exhibit a bluer hue, suggestive of ongoing star formation. The galaxy is relatively isolated, showing no signs of immediate major mergers, although there might be minor disturbances, suggesting possible past interactions or accretion events.
