The galaxy presents an elliptical morphology, exhibiting a largely smooth light distribution. It appears moderately round, displaying only a slight deviation from a circular shape. There is no indication of any ongoing major merging activity. The galaxy exhibits a red-shifted spectral signature, indicative of its recession velocity and distance. Overall stellar mass is estimated to be quite high. The star formation rate appears to be very low, suggesting that the galaxy is likely a quiescent system.
