This galaxy exhibits a disk-like morphology seen nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring a portion of the central bulge. The central region presents a bright, concentrated luminosity profile, possibly indicating the presence of an active galactic nucleus or a dense stellar population. There are hints of a faint, extended halo or disk component beyond the dust lane. The color distribution suggests potential variations in stellar populations within the galaxy, with redder hues along the dust lane and potentially bluer colors emanating from the central region. The disk appears relatively smooth in texture. The overall morphology suggests a spiral or lenticular galaxy with significant dust obscuration. Indications of minor disturbances are potentially present. 
