The galaxy appears as a fairly smooth, elliptical-like structure, exhibiting a high degree of radial symmetry. Its light profile suggests a concentrated central bulge that smoothly transitions into a more diffuse halo. The color distribution is predominantly yellow-reddish, hinting at an older stellar population. A lack of distinct spiral arms or prominent dust lanes implies a relatively quiescent state with likely low current star formation. Overall, the galaxy seems to be a well-formed, mature system.
