The galaxy presents as a largely featureless, elliptical-like structure with a smooth, concentrated light profile. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the center, the color transitions to a slightly redder tone in the surrounding halo, suggesting a mix of older stars and a possible presence of dust. There is no clear evidence of spiral arms or a distinct disk component. The overall morphology points towards a quiescent system with little to no current star formation activity, although a very small amount is possibly present. The galaxy appears relatively isolated with no signs of major disturbances or ongoing mergers.
