The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in intensity outward. There is a subtle color gradient, with a slightly yellower hue dominating the central region which is likely due to a higher density of older stars. Fainter, bluer regions are observed in the surrounding areas, possibly indicating a sparse population of younger, hotter stars. No distinct spiral arms or prominent dust lanes are visible. The overall impression is of a relatively quiescent system with little ongoing star formation. There may be some minor disturbance in the galaxy's structure, although no major mergers are indicated in the image.
