The galaxy presents as a spiral, observed at a moderate inclination angle. Its morphology indicates well-defined spiral arms extending from a central bulge. These arms display a primarily tight winding pattern, with the estimated arm count usually around two. The galaxy appears slightly asymmetrical, potentially indicating minor gravitational interaction or tidal disturbances, or perhaps asymmetries in the galactic disk itself. The bulge is moderately sized relative to the disk. A weak bar structure seems to exist at the center of the galaxy. Patches of intense star forming regions can be inferred within the arms due to the light, indicative of active stellar formation. The core of the galaxy is a bright, concentrated region, indicating high stellar density.
