The galaxy presents as a smooth, elliptical morphology with a moderately elongated shape. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. Moving outward from the center, the light gradually diminishes with no distinct spiral arm structures visible. There are subtle color variations across the galaxy, with the central bulge appearing slightly redder and the outer regions exhibiting a bluer hue, hinting at possible differences in stellar populations. The overall appearance indicates a relatively evolved system. There is a slight distortion and asymmetry on its edges, suggesting potential gravitational interactions. The galaxy seems to have undergone a minor merging event that has disturbed its structure.
