The galaxy appears to be a spiral galaxy viewed at an intermediate angle. The central bulge is visible, though not particularly dominant, and exhibits a relatively smooth, concentrated luminosity profile. Faint spiral arms are present and traceable extending outward from the central region, contributing to its disk-like morphology. The arms are not tightly wound. There's a slight hint of asymmetry in the outer disk. It is light blue overall, which indicates an intermediate star formation rate. The central region does not appear to be obscured by dust, and the overall structure suggests minimal recent merger activity, with the bulk of the galaxy remaining relatively undisturbed.
