The galaxy presents as a relatively face-on spiral galaxy with a prominent central bulge. The bulge appears smooth and bright, exhibiting a concentrated luminosity profile. Spiral arms are faintly visible, possessing a somewhat flocculent structure, with subtle blue-ish star formation regions interspersed within. There is a slight indication of asymmetry in the outer disk region, perhaps due to minor tidal interactions. The overall color suggests a population that is predominantly older stars, but there is also evidence of ongoing, albeit subdued, star formation activity.
