This galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge, roughly ellipsoidal, dominates the galaxy's core. The bulge exhibits a yellowish-orange hue, which could indicate an older stellar population. Fainter, bluish light is observed along the edges of the disk, potentially suggesting the presence of younger, hotter stars and regions of ongoing star formation. There's a slight asymmetry in the distribution of light within the disk, with a hint of a warp or subtle tidal disturbance on one end. Overall, the galaxy appears relatively undisturbed.
