The galaxy presents as a moderately sized, disk-shaped structure exhibiting a distinct color gradient. The central region appears concentrated and exhibits a yellow-orange hue, suggestive of an older stellar population. Moving outward from the center, the galaxy displays a transition toward bluer colors along its visible disk. The galaxy's overall form appears relatively undisturbed, with no immediately obvious signs of a major ongoing merger. However, subtle irregularities may indicate minor gravitational interactions or internal structures. The galaxy's axial ratio suggests that it is observed at a significant inclination relative to our line of sight.