The galaxy presents as a relatively smooth, elliptical structure. Its shape is noticeably elongated, with a high degree of roundness as opposed to being cigar shaped. The central bulge appears bright and concentrated, with a yellow hue, suggesting an older stellar population. The outer regions exhibit a gradual decrease in luminosity and bluer color, possibly indicating some ongoing or recent star formation. There's no clear evidence of spiral arms or significant disturbances, such as those caused by a major merger, although there might be some minor asymmetry. The overall morphology suggests an intermediate stage in galaxy evolution, possibly transitioning toward a more quiescent state.
