The galaxy presents as an elliptical morphology, appearing largely smooth and featureless in this image. The galaxy exhibits a concentrated central bulge which presents with a yellow hue, suggesting a population of older stars. A slight elongation is visible in the shape, though it is generally round in appearance. The overall color gradient shifts from a more yellow center to a slightly bluer halo, which may indicate the presence of a small amount of younger stars in the outer regions, but is likely dominated by older stellar populations. There does not appear to be any significant disturbance or merger activity presently affecting the galaxy's structure.
