The galaxy presents as an edge-on spiral. The central bulge is prominent, displaying a yellowish-orange hue suggesting a population of older stars. The disk is observed as a thin band extending outwards from the bulge, appearing relatively smooth and lacking distinct spiral arm structures. The disk exhibits a slight blueish tint. The overall morphology indicates minimal ongoing star formation and a high degree of inclination with respect to the observer's line of sight. Possible minor disturbances in the disk may exist, but it is hard to tell for sure. The bulge's shape appears to be more rounded.
