The galaxy presents as an elongated, cigar-shaped structure. A central bulge with a yellow-orange hue dominates the galaxy's core. The luminosity appears to decrease smoothly from the center outwards, suggesting an older stellar population concentrated in the core. Surrounding the bulge, faint, bluish extensions are visible along the major axis. These extensions, potentially spiral arm fragments, hint at some ongoing star formation activity, albeit subdued. Overall, the galaxy appears relatively undisturbed.
