The galaxy presents as a moderately bright, somewhat elliptical object. It appears to have a prominent central bulge with a high degree of central concentration. The outer regions of the galaxy fade gradually, showing a smooth profile with what may be a very faint and diffuse disk. There is no clear spiral arm structure visible; the light distribution is fairly smooth and featureless. The galaxy exhibits a general blue-white coloration, suggesting the presence of some young stars, although the overall color appears relatively evolved, hinting at a more quiescent star formation rate. The apparent elongation suggests it is an elliptical or lenticular galaxy, viewed close to face-on but with some degree of inclination. There is no obvious evidence of a major merger or tidal disturbance, though there may be minor disturbances present. Overall, the galaxy seems to be a relatively regular and undisturbed system.
