The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The central region displays a bright, yellowish hue, indicative of an older stellar population. Fainter, bluer regions are interspersed throughout the galaxy. The galaxy is moderately luminous. It appears relatively isolated, showing no strong visual signs of major tidal disturbance or ongoing merger activity, though there is minor asymmetry that may suggest a past interaction. The overall structure is largely featureless, lacking prominent spiral arms or a defined dust lane. The object's shape deviates slightly from perfectly round, appearing somewhat elongated. Based on the observed color and morphology, it appears to be a mature system with a relatively low rate of star formation.
