The galaxy presents as a somewhat smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outward from the center, the light intensity gradually diminishes, forming a diffuse halo. The overall shape is elongated, deviating from a perfect sphere, with a possible faint disk-like structure that is difficult to resolve. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy displays a yellowish-orange hue throughout, which indicates an older stellar population with minimal ongoing star formation. There are no signs of major mergers or tidal disruptions. Minor disturbances cannot be ruled out. The galaxy is of significant mass and absolute magnitude.
