The galaxy appears as a moderately luminous, elongated structure. Its overall morphology is smooth, showing no evidence of spiral arms or a prominent disk. The light distribution suggests an elliptical or lenticular morphology. There is a slight central concentration of light, potentially indicating a core region. The galaxy exhibits a color gradient, with the central region appearing more reddish-yellow and the outer regions subtly bluer, which may indicate varying stellar populations or dust distribution. There is no obvious sign of active galactic nucleus activity or ongoing major merger events. The overall impression is that of a relatively evolved and quiescent system.
