The galaxy presents as a single, centrally concentrated light source. It exhibits a generally smooth morphology, lacking prominent spiral arms or distinct features. The galaxy appears roughly elliptical or spheroidal. There is a slight color gradient visible, with a central region exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions appear somewhat bluer, possibly due to younger stars. Overall, the galaxy's structure is well-defined and coherent. The presence of a high degree of smoothness suggests that the galaxy has undergone significant dynamical evolution. There is no indication of any recent or ongoing major merging events, or any significant disturbance within the galaxy’s overall structure.
