The galaxy presents a largely smooth and rounded morphology. The central region exhibits a bright, concentrated bulge, indicative of an older stellar population, which is suggested by the yellowish hue. Faint, disk-like structures can be tentatively identified extending away from the central bulge. There appears to be some minor disturbance within the main disk of the galaxy.

The overall color suggests a relatively low specific star formation rate. The observed features are consistent with a massive galaxy, likely with only a few stars being actively formed at any given time. 
