This galaxy appears to be a relatively face-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting an older stellar population and a lack of significant dust obscuration. The spiral arms are not sharply defined and exhibit a somewhat flocculent structure. Their color is slightly bluer than the central bulge, indicating the presence of younger, hotter stars. There's a hint of disk structure with faint spiral arm features, which suggests it could be an intermediate type spiral. The arms display some signs of recent or ongoing star formation, but this activity appears to be modest, and not exceptionally vibrant. The overall structure suggests a galaxy that has been relatively undisturbed, although there's very slight evidence of potential minor interaction or internal disturbances.
