The galaxy presents as an edge-on spiral type. A distinct dust lane is not readily apparent, however the galaxy's bulge appears slightly obsecured as if behind a darker region suggesting a potential dust component in the galactic plane. The central bulge is moderately bright, though without a highly concentrated central nucleus visible in this resolution. Faint, diffuse extensions are observed beyond the central region and within the plane, suggestive of spiral arms although those are difficult to resolve given the orientation. There is no sign of major mergers, although there is a minor amount of asymmetry/disturbance to the light along the plane. The central bulge appears slightly elongated, with a more rounded shape, which could imply moderate rotation and an established structure. Based on the coloration, the galaxy appears to have a significant population of older stars, with some ongoing star formation.
