The galaxy presents as a somewhat elliptical object with a bright, relatively smooth core. The light distribution suggests a gradual decrease in intensity from the center outwards. A faint disk-like structure might be present, though it isn't sharply defined. There is a subtle hint of asymmetry or disturbance in the outer regions. Some faint, wispy structures are suggested, but they are not distinct enough to be clearly classified as spiral arms or tidal tails. Overall, the galaxy appears relatively undisturbed, though a minor interaction cannot be entirely ruled out. The color gradient from the center to the outer edges suggests a potentially varied stellar population, with possibly younger, bluer stars concentrated in the disk region.
