The galaxy presents as a largely featureless, elliptical-like object with a smooth light distribution. It exhibits a concentrated central region that appears brighter and more yellowish in color, suggesting a higher density of older stars. Moving outward from the center, the light gradually diffuses, transitioning to a slightly redder hue. There is no clear evidence of spiral arms or distinct structures such as dust lanes. The overall appearance indicates a galaxy in which star formation is likely quiescent, possibly due to its morphological type or the depletion of gas reservoirs. There is a very slight hint of disturbance in the outer halo, but this is very low and needs further investigation.
