The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge and contributing to the reddening of light observed along the galactic plane. The central region appears yellowish-white, possibly indicating a population of older stars. The outer regions of the disk show bluer coloration, suggesting the presence of ongoing star formation. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or recent merger events. The bulge appears rounded, without significant boxiness. There are some signs of minor disturbance in the disk. Overall, this is a relatively massive galaxy with low star formation activity.