The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall form appears elliptical, exhibiting a high degree of roundness in its isophotes. There is a suggestion of a merging event, likely a major disturbance or merger, given the galaxy's slightly disturbed appearance. The primary body displays a notable color gradient, with a redder hue towards the center and a bluer tint in the outer regions. This color variation potentially indicates variations in stellar populations across the galaxy, with older, redder stars dominating the core and younger, bluer stars populating the outskirts. The galaxy's moderate redshift suggests it is located at a significant cosmological distance. The estimated size indicates it is a large galaxy.
