The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge, appearing a warmer yellow hue, with a gradual decrease in intensity towards the outer regions. The outer regions exhibit a cooler, greenish color suggesting a population of relatively young stars. A faint, diffuse halo surrounds the central region, extending outwards in a roughly spherical shape. There are no apparent spiral arm structures, although a very subtle disc-like feature is suggested. The overall morphology indicates a system with a dominant spheroidal component. Possible minor disturbances can be noticed in the galaxy's shape, but there is no clear sign of major ongoing merging activity. The galaxy displays an intermediate redshift, indicating a relatively significant distance from the observer.
