The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure with a high degree of central concentration. The light profile appears to be largely dominated by older stellar populations, based on the color gradients observed. It exhibits a moderate redshift, indicating a considerable distance. It is likely a galaxy with a small-to-moderate mass. Star formation appears relatively quiescent. The galaxy displays a slight elongation, with an axial ratio suggestive of an E4-E6 classification on the Hubble sequence. There is no evidence of tidal features, strong dust lanes, or other signs of recent merger activity.
