The galaxy appears to be an elliptical type, exhibiting a generally smooth, featureless morphology with a high degree of central concentration. It shows a slight elongation, trending toward a cigar-like shape. The light profile suggests an older stellar population, with a color gradient trending redder toward the core, indicative of less active star formation in the central regions. Faint bluer hints are observed in the outer regions of the galaxy. There is no evidence of a major merger or significant tidal disturbances, although a minor interaction or disturbance cannot be ruled out given the slight asymmetry present. The galaxy exhibits a small angular size on the sky, consistent with its considerable distance. Overall, the galaxy presents as a relatively evolved and quiescent system.
