This galaxy exhibits a largely smooth morphology. It presents a centrally concentrated, bright core that fades gradually into its outer regions. The light distribution suggests an elliptical shape with a high degree of roundness. There is no evidence of prominent spiral arms or a distinct disk structure. Faint, diffuse light extends outwards from the main body, but there are no apparent signs of ongoing mergers or tidal disturbances. The galaxy's overall color appears to be on the redder side, suggesting a population of older stars. The lack of distinct features implies a relatively quiescent star formation rate.
