The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on from our vantage point. There is a prominent central bulge, exhibiting a smooth, somewhat rounded morphology. The bulge appears yellowish in color, suggesting a population of older stars. The galactic disk extending outwards from the bulge displays a more diffuse and irregular texture, with some indication of dust lanes and possibly some faint spiral arm structure. The overall color of the disk seems bluer than the bulge, hinting at the presence of younger, hotter stars within the disk. There are no obvious signs of ongoing major mergers or strong tidal disturbances in the immediate vicinity, though there may be some minor asymmetry in the outer regions of the disk on one side.
