The galaxy presents a smooth, elliptical morphology. It appears to be a spheroid-dominated system, with a notable lack of discernible spiral arms or a prominent disk structure. The galaxy exhibits a radial color gradient, transitioning from a yellowish, concentrated core to a bluer outer halo. The overall structure suggests a relatively quiescent galaxy with low rates of star formation, with the bulk of the stellar population likely composed of older stars. There is no evidence of a recent or ongoing major merger event or significant tidal disturbances, implying a relatively isolated evolutionary path. The galaxy has a moderate redshift.
