The galaxy appears to be an elliptical type, exhibiting a smooth, generally featureless morphology. The overall shape is approximately round, with no discernible spiral arms or bar structures. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer edges. There may be some indications of minor disturbance in the light distribution, hinting at a possible interaction or past merger event. Color gradients suggest older stellar populations dominate, exhibiting reddish hues with subtle blueish regions, possibly indicating areas of residual, low-level star formation. Based on the observed characteristics, it is likely a relatively massive galaxy with a suppressed star formation rate and high stellar mass.
