The galaxy presents as an edge-on spiral, exhibiting a notable disk structure. The central bulge is prominent, appearing relatively smooth and elongated along the major axis of the galaxy. There is no clear bar structure visible. The dust lane, typical of edge-on spirals, is subtle but detectable, causing slight attenuation in the light from the disk. Star formation appears to be occurring, given the slightly bluish tint. Overall, the galaxy presents as a regular, well-formed disk galaxy with no obvious signs of significant interaction or major disturbance. The bulge appears to be more rounded. 
