The galaxy presents a generally smooth morphology, appearing largely elliptical in shape with a high degree of central concentration. The light distribution suggests a dominant spheroidal component. There is a discernible color gradient, with the central region exhibiting a yellowish hue, possibly indicating an older stellar population, while the outer regions appear bluer. The overall structure appears undisturbed, without any obvious signs of major mergers or tidal features. There are no apparent spiral arm structures or a pronounced disk. There may be some minor disturbances or irregularities in the outskirts, but they are subtle. The galaxy's color suggests it may have low star formation, with a significant fraction of older stars.
