The galaxy presents as a largely featureless, elliptical morphology. There is a high degree of central concentration of light, with a smooth, diffuse halo surrounding the core. Color gradients appear subtle, with the core exhibiting a slightly yellower hue compared to the outer regions. There is no indication of spiral arms, dust lanes, or any significant tidal disturbances suggesting recent major merger events. The overall symmetry suggests a relaxed system likely dominated by an older stellar population. Close inspection reveals a very slight elongation, but its aspect ratio is fairly close to unity, and its overall shape is considered to be moderately rounded. Evidence of current significant star formation is not apparent in the image.
