The galaxy presents a generally smooth, elliptical morphology. There is a concentration of light towards the center, suggesting a central bulge component. The light distribution appears relatively symmetric. There is a hint of a slight disk, or at least some non-smooth features, surrounding the central region. No prominent spiral arm structures or bar features are immediately apparent. There is no evidence of a major merger event in the image, but there may be some slight disturbance in the galaxy's shape. The colors suggest a population of older stars, particularly in the central bulge, but there is also some bluer light in the outer regions that may indicate more recent star formation activity, although the colors are difficult to discern. The galaxy exhibits a somewhat round shape, with a minor deviation from perfect sphericity.
