The galaxy presents as an edge-on spiral, exhibiting a distinct flattened disk structure. The central bulge appears prominent and rounded, with a bright, concentrated luminosity suggesting a significant stellar population. The disk component displays a relatively smooth texture, with minimal signs of resolved star-forming regions or dust lanes in the visible bands. Overall, the galaxy appears moderately luminous and relatively massive, with a low rate of current star formation. Indications are that it is not currently undergoing any significant merger activity.