The galaxy presents as a late-type spiral system, viewed nearly edge-on. A prominent dust lane is visible, bisecting the galactic disc and obscuring portions of the central bulge. The bulge appears relatively bright and is centrally concentrated, exhibiting a smooth, rounded morphology. The overall color of the bulge and disc is generally yellowish, suggestive of a population of older stars, with possible areas of ongoing star formation. There appear to be faint spiral arms extending from the central bulge to the edge, however, the outer regions of the disc seem somewhat irregular and asymmetric. Based on the color and morphology, the galaxy is likely to have a stellar mass between 10^10 and 10^11 solar masses, with a low to moderate star formation rate. There are no clear signs of any major ongoing mergers or tidal interactions. Minor disturbances and asymmetries in the disc structure may suggest past minor interactions.
