The galaxy appears as a somewhat elliptical, centrally concentrated object. The core exhibits a distinct yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, a subtle transition to a greenish halo is observable, possibly indicating the presence of a younger stellar population. The overall structure appears relatively smooth with no apparent spiral arms or distinct features. The galaxy is moderately luminous and shows no signs of recent major merger events. There may be some minor asymmetry, suggesting past or ongoing minor interaction or disturbance, however this cannot be determined from this image alone. The isophotes are rather regular and smooth.
