The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions gradually into a more diffuse halo. The overall color profile suggests a population of older stars, with a subtle reddening toward the core, which may indicate a higher concentration of dust or older, redder stars. There are no prominent spiral arms or dust lanes visible, lending further credence to its classification as an elliptical galaxy. The galaxy exhibits a high degree of radial symmetry, suggesting a dynamically relaxed system. There is very little evidence of active star formation, with the galaxy displaying a generally quiescent appearance. The faint, extended halo suggests some tidal interactions in the past but little or no ongoing merger activity. The galaxy appears roughly circular in shape, with a slight elongation along one axis.
