The galaxy appears as a single, somewhat elliptical object. The light is primarily distributed evenly, exhibiting a smooth profile, with the highest concentration of luminosity at its center, with luminosity gradually decreasing outward. There is a slight elongation to its shape, but it generally appears quite round. The galaxy exhibits a color gradient, with a reddish-orange hue dominating, but with hints of greenish-yellow present in the outer regions. There is no evidence of spiral arms or a prominent disk structure. There is no obvious evidence of ongoing major merger activity, though there might be minor disturbances present in the galactic structure.
