The galaxy presents as an edge-on spiral, with a notable dust lane bisecting its major axis. The central bulge is prominent and appears relatively smooth with a slightly boxy shape. Faint extensions are visible beyond the central bulge, indicative of a disk. The color profile suggests a central concentration of older stars. Minimal disruption is apparent, suggesting the galaxy has not undergone any recent major merger events. Star formation seems to be occurring, although at a modest rate. The overall morphology of the galaxy places it within the mass range of a typical spiral.
