The galaxy presents a flattened, elliptical morphology when viewed from our observational perspective. A discernible central bulge exhibits a concentrated, yellowish-white hue, suggesting a population of older stars. Fainter, diffuse material extends outward from the bulge. A subtle disk-like component seems present; slightly bluer hues towards the outer edges indicate the presence of younger stars. There appears to be limited discernible spiral arm structure. Overall, the galaxy appears relatively undisturbed, exhibiting a smooth, integrated light profile. There is no significant morphological evidence of a major merger event.
