The galaxy appears as an elliptical-type system, exhibiting a smooth, centrally concentrated morphology. The light profile suggests a bulge-dominated structure, with the isophotes becoming increasingly elliptical towards the outer regions. The core displays a yellowish hue, potentially indicative of an older stellar population. There's a subtle blue gradient extending outward from the core, possibly suggesting the presence of younger stars in the outer regions. The overall structure appears relatively undisturbed, lacking any clear signs of major mergers or tidal disruptions. However, slight asymmetry is observable, which could be indicative of a minor interaction or internal dynamics. There are no indications of prominent spiral arms or a well-defined disk structure.
