The galaxy presents as a centrally concentrated system with a smooth, diffuse morphology. A luminous, yellowish core dominates the galaxy's central region. The core's light appears to fade gradually outward into a less structured, more diffuse halo. There may be weak spiral arm features, evidenced by the subtle blueish colorations extending away from the central core. The overall shape appears elliptical, but the hint of asymmetrical blue extensions could suggest some disc-like structure. Based on its color indices, the galaxy exhibits characteristics of a relatively evolved system with a moderate rate of star formation. No apparent signs of major mergers or significant tidal disturbances are evident, though there are suggestions of minor perturbations in its overall structure.
