The observed galaxy presents as an edge-on spiral, exhibiting a distinct disk structure. The bulge appears elongated and relatively faint, with the majority of light concentrated along the plane of the disk. There is a noticeable dust lane that bisects the galaxy along its major axis, causing obscuration of light from regions behind the disk. The dust lane appears darker and more prominent towards the central region of the galaxy, gradually fading towards the outer edges. The disk appears relatively smooth, exhibiting no major signs of recent or ongoing major merger events. No tidal tails or other significant disturbances in the surrounding halo are evident. The overall color profile suggests a relatively quiescent star formation rate, with a population of older stars dominating the visual light output. The integrated color appears redder than typical spiral galaxies, possibly due to the obscuring effects of the dust lane and the lack of intense star-forming regions. The galaxy's apparent size is relatively small, suggesting a moderate distance.
