The galaxy presents as a centrally concentrated elliptical morphology, with a smooth light distribution. It has a notably rounded shape, lacking any apparent spiral arm structures or significant disk features. The core exhibits a yellowish hue, suggestive of an older stellar population. The galaxy gradually fades in luminosity from the center to the edges, indicating a decreasing stellar density gradient. There is no evidence of significant ongoing star formation, tidal disturbances, or mergers. The overall appearance suggests a relatively quiescent system, potentially a massive elliptical galaxy at intermediate redshift.
