This galaxy presents a largely smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decline in luminosity outwards. The core region exhibits a yellowish hue, which could indicate an older stellar population and less ongoing star formation. There is a possible disk like feature and some signs of minor disturbance, as indicated by the non-uniform distribution of light in the outer regions. The overall color suggests that the galaxy is likely undergoing passive evolution. The object has an approximate half-light radius on the order of 7 kpc.
