The galaxy presents as a largely featureless, smooth object with an elliptical morphology. There is a subtle color gradient, transitioning from a yellowish central bulge to a greenish outer region. The light distribution suggests a concentration of older stellar populations in the bulge, with a possible indication of a more recent, albeit low, level of star formation occurring in the surrounding disk. The overall shape is not perfectly round, displaying a slight elongation. There is no apparent evidence of tidal tails, streams, or major morphological disturbances indicative of recent major merger activity. Subtle asymmetry in the outer regions might suggest a minor interaction or disturbance.
