The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent dust lane bisects the galaxy's bulge, obscuring the central regions and contributing to the apparent reddening. The bulge appears relatively smooth and elongated, with a brighter concentration toward the center. The disk component extends outwards from the bulge, displaying a fainter, more diffuse distribution of light. The outer regions of the disk are somewhat irregular and uneven, possibly indicating tidal interactions or ongoing accretion events. There is an overall reddish tint in the light, suggestive of a population of older stars and dust obscuration. No clear spiral arm structure is discernible, likely due to the edge-on viewing angle.
