The galaxy presents a face-on spiral morphology. The central bulge appears prominent and has a smooth, concentrated luminosity profile, indicating a possible classical bulge structure. The spiral arms are well-defined and exhibit a moderately tight winding. There appears to be a relatively high degree of symmetry in the overall structure. Dust lanes are subtly visible within the spiral arms. Based on the spiral arm structure, it is probably a barred spiral galaxy, but the bar appears faint, with only a moderate intensity. The galaxy displays a range of colors, with the bulge showing a yellow tint while the spiral arms are bluer, suggestive of differing stellar populations. The ratio of the minor axis to the major axis indicates that the galaxy is not perfectly circular, showing a slight ellipticity. There appear to be no major disturbances in the morphology, so there is no visible evidence of recent major merging events, although some minor disturbances may be present. Star formation is likely present within the spiral arms. 
