The galaxy presents as a singular, relatively smooth object with a concentrated central bulge. The color gradient transitions from a yellowish-white core to a faint greenish-blue outer region, suggesting varying stellar populations. The shape appears approximately elliptical or lenticular, lacking any obvious spiral arm structures. There's no readily apparent evidence of a major ongoing merger or significant tidal disruption. There might be a hint of minor asymmetry or disturbance in the outer regions, but it's subtle. The overall light distribution indicates a relatively evolved system with a dominant, older stellar population.
