The galaxy appears to be a spiral galaxy viewed at a moderate inclination. The central bulge is clearly visible and appears to be a relatively smooth, concentrated structure. Faint spiral arms extend from the central region, displaying a somewhat flocculent structure. The arms exhibit a subtle bluish hue, which suggests ongoing star formation within them. The overall structure indicates a relatively late-type spiral classification, likely an Sc type. There is some visual evidence of minor disturbances, but overall the disk appears relatively undisturbed. The galaxy displays a fairly well-defined central region, with a gradual decline in surface brightness as one moves towards the outer regions. The axial ratio of the galaxy indicates a moderate degree of flattening, consistent with a spiral structure.
