The galaxy presents as an edge-on spiral, with a prominent central bulge that appears largely spheroidal and exhibits a yellowish hue, likely indicating an older stellar population. The disk is highly inclined with respect to our line of sight, obscuring much of its detailed structure. There's a possible dust lane visible along the equatorial plane bisecting the galaxy. The outer regions of the disk show a bluer tint suggesting the presence of younger stars, although the resolution is insufficient to resolve individual star-forming regions. Overall, the galaxy has an elliptical appearance due to the edge-on orientation, with a smooth, though somewhat diffuse, profile. There are not apparent signs of ongoing major mergers or tidal distortions, though there is a smaller secondary light source on one edge of the galaxy. The disk terminates relatively abruptly, as if truncated.
