The galaxy presents as a spiral, observed at an angle between face-on and edge-on. There is a central bulge that appears moderately sized and is slightly elongated. Spiral arms are present, with a somewhat tightly wound structure. Evidence suggests at least two spiral arms originating from the bulge. The outer disk exhibits flocculent structure, with noticeable star formation regions appearing as brighter, bluer patches. There is a possible weak bar structure present within the bulge. The galaxy appears relatively isolated, showing no signs of significant tidal disturbances or ongoing mergers. The overall color profile suggests a mixed stellar population, with older, redder stars concentrated in the bulge and younger, bluer stars populating the spiral arms. The overall structure seems relatively undisturbed and indicative of ongoing spiral arm formation.
