The galaxy presents as an elongated, lenticular structure, exhibiting a distinct edge-on disk morphology. The central bulge appears prominent and smoothly distributed. The color gradient suggests a slightly older stellar population within the bulge.  Faint hints of a disk extend outwards from the central region. A slight asymmetry is suggested in the outer regions, possibly indicating some minor gravitational interaction or internal disturbance, though the overall structure appears largely undisturbed. No prominent dust lanes or active star-forming regions are readily apparent in this optical image. 
