The galaxy presents as a largely featureless, elliptical-like structure, exhibiting a smooth light distribution. The primary color appears to be a yellow-orange hue, suggesting an older stellar population with a lower rate of current star formation. There is a slight asymmetry in the light distribution, possibly indicating a minor interaction or internal disturbance. A faint, blueish patch is observed on one side of the galaxy, potentially indicating a region of more recent, but modest, star formation. The overall shape appears to be close to circular. There is a noticeable absence of spiral arms or a distinct disk structure. Evidence of major merging events is not readily apparent.
