The observed galaxy appears to be a spiral galaxy, viewed edge-on from our vantage point. It exhibits a prominent central bulge, seemingly spherical in projection, and a relatively thin disk. The disk presents a smooth appearance, with little to no resolved structure such as spiral arms or distinct dust lanes visible. The outer regions of the disk fade gradually into the background sky. There are no obvious signs of ongoing mergers or tidal interactions, but there is some minor disturbance. The overall color is slightly redder, suggesting an older stellar population and a lower rate of star formation within the galaxy. The galaxy has a slightly elliptical shape.
