This galaxy appears to be a relatively smooth, centrally concentrated system. The light distribution suggests an elliptical morphology, with a gradual decline in brightness from the core outwards. There's a subtle color gradient, with the central region exhibiting a slightly yellower hue, possibly indicating a population of older stars, while the outer regions may have a bluer tint, suggestive of some ongoing or recent star formation activity. The overall structure is fairly undisturbed, without any significant signs of tidal features or major asymmetries indicative of recent mergers. The galaxy is moderately luminous.
