The galaxy presents as a single, concentrated body with a smooth, elliptical morphology. There is no readily apparent disk structure or spiral arm formation. The light distribution appears to be centrally concentrated, fading gradually towards the outer edges. The core exhibits a yellowish hue, suggesting a population of older stars, while the outer regions show a slight bluer tint, possibly indicating younger stellar populations. The overall color suggests a relatively passive galaxy with moderate star formation. There is no obvious evidence of ongoing merging activity or major disturbances in the galaxy's structure. The shape appears generally round.
