The galaxy presents as an elongated, spindle-shaped structure. It exhibits a central bulge that is noticeably brighter and appears to be more densely packed with stars. The color of the bulge tends toward the yellower end of the spectrum. Extending outward from the bulge are fainter, more diffuse structures that likely represent the galactic disk. The disk appears relatively smooth, lacking prominent spiral arm features or significant dust lane obscuration. The overall color gradient suggests a population of older stars, with a lower rate of ongoing star formation across the galaxy as a whole. The galaxy's shape indicates it is viewed at an oblique angle, not face-on. There might be signs of disturbance from a minor merger on one side of the galaxy, or possible irregular features.