The galaxy presents as a relatively bright, centrally concentrated object with a slightly elongated, elliptical morphology. The core exhibits a yellow-orange hue, suggestive of an older stellar population. Moving outward from the core, the light transitions to a bluer, less intense halo, possibly indicating the presence of a younger stellar population or ongoing star formation in the outer regions. The overall structure appears relatively smooth, with no immediately obvious signs of spiral arms or major disturbances due to interactions or mergers, although some minor asymmetry cannot be ruled out. The distribution of light suggests the galaxy is more closely described as an elliptical or lenticular type.
