The galaxy presents as a flattened, disk-shaped system, viewed nearly edge-on. A prominent central bulge dominates the core, exhibiting a smooth, bright, yellowish-white luminosity gradient indicative of an older stellar population. This bulge appears to be slightly elongated along the major axis of the disk.

The galactic disk extending from the bulge shows a fainter, more diffuse distribution of light, with hints of some internal structure. The color of the disk shifts towards a reddish-orange hue, possibly due to the presence of dust obscuration or a redder stellar population compared to the bulge. The disk appears to have consistent coloration throughout, indicating a relatively uniform distribution of star formation or dust content. There are no apparent spiral arm features or knots of active star formation readily visible in the disk. The overall shape of the galaxy is relatively smooth and undisturbed. The galaxy is fairly massive based on its luminosity profile and size.
