The observed galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge dominates the light profile, exhibiting a smooth, rounded morphology. The bulge appears yellowish-white, suggesting a population of older stars. The disk is comparatively faint and elongated, spanning approximately 5 kiloparsecs. Due to its edge-on orientation, discerning any spiral arm structure is not possible. The overall color suggests that it is a relatively massive galaxy, with a stellar mass possibly around 10^10 solar masses. There is no obvious signature of ongoing major merger activity. There are a few minor areas of blue light in the disc that suggest it may be in the midst of a very low star formation rate. 
