The galaxy exhibits a prominent disk structure, observed at a relatively face-on orientation. Well-defined spiral arms emanate from the central region, displaying a two-armed morphology. The winding of the spiral arms appears to be intermediate, neither tightly wound nor loosely structured. The central bulge is moderately sized, contributing a noticeable but not dominant fraction of the overall galactic luminosity. The color distribution suggests ongoing star formation, particularly within the spiral arms. There is a hint of a possible weak bar feature spanning the galaxy's core, but it is not a prominent characteristic. The overall structure appears relatively undisturbed with a relatively large, faint halo, lacking any signs of major merging events or significant tidal disruptions. The overall size is of average size.
