The observed galaxy presents as a luminous, relatively smooth system with a generally elliptical morphology, displaying a moderate degree of roundness. There may be a slight tidal disturbance or early stage merger occurring. The galaxy's overall color is slightly red. This suggests a moderate presence of older stellar populations and relatively diminished ongoing star formation. The central region shows high intensity, which gradually fades towards the edges, with an estimated size of around 8 kpc. A possible secondary nucleus or concentration is suspected, either another galaxy beginning to merge or a region of very high star formation.
