The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing a yellowish-orange hue. The color suggests a dominant population of older stars. Moving outward from the core, the intensity of light diminishes gradually. The outer regions of the galaxy display a faint, diffuse glow, tinged with a slightly bluer color than the core which indicates some, but not very much, younger star formation. No distinct spiral arms or bar structures are discernible. The overall appearance suggests a relatively evolved system, potentially in a late stage of its evolutionary process. There is no evidence of any ongoing major mergers, although some minor disturbances cannot be ruled out.
