The galaxy appears to be a spiral type, viewed at a slight angle. A prominent central bulge is observed, displaying a yellowish hue, which suggests an older stellar population dominating the core. Diffuse spiral arms extend outwards from the bulge. These arms exhibit a bluer color, indicative of ongoing star formation regions. The arms are somewhat patchy and not very tightly wound. There does not appear to be a strong bar-like structure. The outer regions of the galaxy fade gradually into the background, with no sharp cut-off observed in the visible light. Overall, the galaxy presents as a relatively undisturbed and evolving spiral system. There seems to be some minor asymmetry in the distribution of light in the disk.
