The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that graduates into a more diffuse halo. The color profile suggests an older stellar population, with a yellow-orange hue dominating the galaxy's light. There is no clear evidence of active star formation or prominent spiral arm structures. The galaxy is mostly featureless in its morphology, with minimal visible disturbances or signs of ongoing merger activity. The shape is somewhere in between round and elliptical, with the major to minor axis ratio is moderate.
