The galaxy presents as a fairly smooth, elliptical-like structure. It appears largely spheroidal in shape with a high degree of central concentration, showing a gradual decrease in luminosity from the core outwards. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a color gradient, with a slightly bluer, possibly star-forming core transitioning to redder hues in the outer regions. There is no indication of major mergers or tidal disturbances in the immediate vicinity. Based on the light profile, it seems to be a relatively evolved galaxy with a significant spheroidal component.
