The galaxy presents as a single, fairly smooth object, lacking any readily discernible spiral arms or bar structure. It appears elliptical in shape, with a high degree of central concentration of light. The core exhibits a yellowish-orange hue, suggesting an older stellar population. There is a gradual decrease in surface brightness moving outwards from the center to the edges of the galaxy. The outer regions present a slightly bluer color, which may indicate a younger stellar population in these areas. No major signs of tidal disturbances or ongoing mergers are apparent based on the galaxy's morphology; however, some minor irregularities may be present upon closer inspection. The object appears to be a relatively undisturbed elliptical galaxy.
