The galaxy presents as a relatively small, disk-shaped structure, observed nearly edge-on. A prominent central bulge dominates the luminosity profile, exhibiting a concentrated, bright, yellowish-white hue, suggesting an older stellar population. The disk component appears as a faint, elongated band extending outwards from the central bulge. There is very little visible texture to the galaxy; it is very smooth. The outer regions of the disk appear somewhat less luminous and have hints of bluer color, potentially indicating the presence of younger, hotter stars. There are no immediately obvious signs of spiral arm structure or prominent dust lanes within the observed portion of the disk. The overall symmetry of the disk suggests a generally undisturbed morphology, though higher resolution data would be needed to confirm the absence of minor interactions or tidal features. 
