The galaxy presents as a centrally concentrated elliptical or lenticular type system, exhibiting a smooth, relatively featureless morphology.  It is characterized by a dominant, spheroidal bulge component that appears largely homogeneous, with minimal dust lane obscuration or prominent star-forming regions discernible. The luminosity profile suggests a gradual decline in brightness from the core outwards, indicative of a well-established stellar population.  A faint, diffuse halo may extend outwards from the main body, but any extended disk-like structure is either absent or faint and viewed nearly face-on. Weak tidal features or distortions are potentially present, however they appear very minor if they are present at all. The galaxy exhibits a color gradient from a yellowish core that fades to redder hues at the edge, suggesting that younger stars are mostly in the core with older stars near the edge.
