This galaxy presents as an edge-on spiral galaxy, characterized by a distinct, flattened disk. The central bulge appears prominent and is centrally concentrated with a relatively smooth texture. The disk shows evidence of some internal structure, though detailed features are difficult to resolve. Dust lanes are likely present within the disk, obscuring some of the light from the stars behind them and contributing to the patchy appearance. The galaxy appears to be relatively isolated, with no obvious signs of a major ongoing merger, though minor disturbances cannot be ruled out.
