The galaxy presents as a somewhat elongated, disk-like structure viewed at an oblique angle. The central region exhibits a concentrated brightness, appearing smooth and yellowish-orange in color, likely indicating an older stellar population. The outer regions appear less defined, with a fainter, somewhat patchy distribution of light. There's subtle evidence of a slightly bluer hue on the periphery, hinting at some ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger or significant tidal interactions.
