The galaxy presents as a centrally concentrated system, generally elliptical in shape. It appears largely smooth, with a notable absence of prominent spiral arms or other distinct features. The central region is significantly brighter and exhibits a yellowish hue, suggestive of an older stellar population. The galaxy's light gradually fades toward the outer edges, forming a diffuse halo. There is a very faint blue tint in the halo, which indicates presence of some younger stars. Overall, the galaxy exhibits a relatively quiescent appearance, indicating a low star formation rate.
