The observed galaxy presents as an edge-on spiral, characterized by a prominent dust lane bisecting the central bulge. The bulge appears smooth and elongated, indicative of a spheroidal structure. Faint, diffuse extensions are visible perpendicular to the major axis, likely representing a faint galactic halo. The disk component exhibits a slight warp or distortion, potentially indicative of past interactions or internal dynamics. A prominent dust lane attenuates light along the disk's midline. The color gradient suggests a stellar population gradient, with the central bulge appearing redder and older, and the outer disk showing bluer hues possibly related to ongoing star formation. The galaxy is relatively compact.
