The galaxy presents as a concentrated, elliptical structure with a smooth, relatively featureless morphology. Its core exhibits a bright, yellowish-white hue, suggesting a population of older stars and a potentially significant contribution from an active galactic nucleus or a dense stellar core. There is a slight color gradient moving outward from the center to a more reddish tint, which may indicate a decreasing age of the stellar population with increasing radius or a larger amount of dust in the outer regions. The galaxy shows no obvious signs of spiral arms or a disk-like structure. There is no evidence of any major ongoing merger events or significant tidal disturbances in the immediate vicinity, giving it the appearance of an undisturbed, evolved system. Its round shape indicates that it does not have a disk-like structure.
