The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits high luminosity, appearing nearly white, suggesting a concentration of older stars. Moving outward from the core, the light gradually fades. Subtle color variations are observable in the outer regions. A slight bluer hue is perceptible, possibly indicating regions of younger star formation, although such regions are not particularly prominent. There is no obvious spiral structure nor any major signs of ongoing merger activity. It presents an overall morphology that would be classified as an elliptical or S0-type galaxy.
