The galaxy presents a primarily smooth morphology with a slightly elongated, disk-like structure observed nearly edge-on. The central region exhibits a bright, concentrated core that is more compact. There's evidence of a disk structure surrounding the bulge. The color distribution indicates a central concentration of older stellar populations, showing a redder hue, while the outer regions appear somewhat bluer, suggesting the presence of younger stars or ongoing star formation. There is some possible minor disturbance to the galaxy's structure. Overall, the galaxy appears relatively undisturbed.
