The galaxy presents as a relatively smooth, disk-like structure with an overall elliptical morphology. The central region is characterized by a bright, concentrated bulge exhibiting a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, a flattened disk structure is observed. This disk displays a subtle color gradient, transitioning towards a slightly bluer tint, indicating the presence of younger stars. The disk shows a slight degree of asymmetry, but overall lacks any readily identifiable spiral arm structure. There's no evidence of significant dust lanes or active star-forming regions easily observed within the resolution of the image. The outer edges of the galaxy fade gradually into the background, indicating a relatively diffuse halo structure.
