The galaxy appears to be a spiral galaxy, viewed at an oblique angle. It exhibits a bright, concentrated central bulge, likely indicative of a significant population of older stars. The disk is relatively smooth, with subtle hints of spiral arm structure. The galaxy's overall color is bluish-white, which could signify the presence of on going star formation. There is a slight asymmetry to the disk, possibly due to a minor gravitational disturbance or interaction. The galaxy appears relatively isolated, with no clear evidence of a major merger. The outer edges of the galaxy have a smooth texture.