The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing largely rounded in shape with a slight elongation. There is a clear central bulge that dominates the overall luminosity profile. The light appears to gradually fade from the center outwards, with no distinct spiral arm structures or features. The galaxy displays a color gradient, with the central region appearing somewhat yellowish-white, indicative of an older stellar population. The outer regions exhibit a more bluish hue, suggesting the presence of younger stars, although this is much less pronounced. There are no obvious signs of ongoing major mergers or tidal disturbances, although a slight asymmetry in the outer halo cannot be ruled out.