The galaxy presents as an elliptical morphology, with an observed redshift indicating it is a distant object. The color indices suggest a population of older stars, giving it a reddish-yellow hue. It exhibits a relatively smooth appearance, with a high concentration of light towards the center. There is evidence of a possible minor disturbance, which could be a sign of a past or ongoing interaction or merger. Its estimated size is approximately 7 kpc in radius, and its calculated stellar mass is quite high. The estimated star formation rate is low, indicating that it is not forming many new stars.
