The galaxy presents as a moderately luminous object at a redshift of approximately 0.28, indicating a considerable distance. It displays an elliptical morphology, appearing largely smooth with minimal visible substructure, suggestive of an early-type galaxy. There is some indication of minor disturbance, potentially due to a past or ongoing interaction, as evidenced by some irregularity in the outer isophotes. The galaxy exhibits a radial color gradient, with the core appearing more yellow than the outer regions, which appear slightly bluer. This color difference may indicate variations in stellar populations, with a higher concentration of older, redder stars in the nucleus and relatively younger, bluer stars in the outer regions. Based on the estimated absolute magnitudes and color, the galaxy likely possesses a substantial stellar mass and a relatively low star formation rate.
