The galaxy appears as a flattened, disk-shaped structure, viewed nearly edge-on from our perspective. There is a prominent central bulge, appearing somewhat elongated along the disk's major axis. The disk itself exhibits a subtle color gradient, suggestive of varying stellar populations or dust obscuration. A faint dust lane is possibly present, bisecting the galaxy along its major axis. No clear spiral arm structure is discernible; however, some irregularity in the disk's light distribution suggests the presence of some internal structure. The galaxy's overall color is relatively red, suggesting a population of older stars or significant dust content. There is little evidence of ongoing star formation, based on the lack of bright blue regions. There is no significant sign of any recent major merger events or tidal disturbances.
