The galaxy presents a primarily smooth and rounded appearance, suggesting an elliptical morphology or a disk galaxy viewed at a significant inclination. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is no distinct spiral arm structure visible. The galaxy exhibits a yellow to slightly reddish hue, implying a population of older stars and a relatively low rate of ongoing star formation. There is a slight suggestion of a faint, disturbed feature that could possibly be a minor merger event, but the galaxy's overall structure is fairly undisturbed. The galaxy appears to be of considerable size and mass, indicative of a large galaxy. 
