The galaxy presents as a moderately bright, elliptical morphology. The object exhibits a concentrated core region, with a gradual decrease in luminosity extending outwards. The overall color profile suggests an older stellar population, with a yellowish-orange hue dominating. There is no evident spiral structure or active star-forming regions observed. Based on the observed features, the galaxy is most likely a relatively massive, quiescent system with a low star formation rate. The general appearance of the galaxy indicates that it is likely a relaxed system which could possibly be undergoing a merger.
