The galaxy presents as an edge-on spiral, with a prominent, elongated disk exhibiting a moderate degree of dust lane obscuration bisecting the central bulge. The bulge appears substantial and moderately bright, exhibiting a smooth texture, indicative of an older stellar population. The disk component shows a gradual fading intensity away from the bulge along the major axis, and a notably thinner profile along the minor axis, confirming the edge-on perspective. There are suggestions of spiral arm structures within the disk, but their visibility is limited due to the viewing angle and internal obscuration. The color profile exhibits a redder central bulge transitioning to slightly bluer hues in the outer disk. The galaxy appears relatively undisturbed with no signs of major merging events, and it exhibits signs of active star formation in the disk. Overall, this object likely represents a late-type spiral galaxy viewed edge-on with moderate bulge prominence and ongoing stellar activity.