The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing nearly circular in projection with a slight deviation towards a more rounded shape. The light profile suggests minimal internal structure, with a high degree of smoothness across the observed surface brightness. The galaxy's core is distinctly bright and yellowish-white, implying a population of older stars dominating the central regions. A subtle color gradient appears to be present, with the outer regions displaying slightly redder hues, potentially indicating either an older stellar population or the presence of dust obscuration at the periphery. There is no apparent spiral arm structure or bar feature visible. There are no obvious signs of recent major merger events. A very slight perturbation is present in the galaxy's halo. Based on its morphological characteristics, this galaxy is likely to be a massive elliptical galaxy at intermediate redshift with subdued levels of ongoing star formation.
