The galaxy presents as a spiral galaxy, viewed at a significantly inclined angle. The galactic disk is not perfectly edge-on, but close enough that detailed spiral arm structure is not easily discernible without further analysis. There is a notable central bulge region, which appears moderately sized relative to the overall disk. The galactic nucleus appears to be a bright, centrally located region indicating likely intense activity. The dust lanes are visible within the disk, obscuring some of the starlight particularly towards the near side of the galaxy. The overall color of the galaxy appears to be a mix of blue and yellowish-white, suggesting a combination of older stellar populations in the bulge and ongoing star formation within the disk. The elliptical shape of the disk is evident, with a major to minor axis ratio estimated to be approximately 2:1. The galaxy appears relatively isolated, showing no obvious signs of major interaction with neighboring galaxies, although there might be some minor disturbances or slight asymmetries in its structure.
