The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light profile. There is little evidence of spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a reddish-orange core indicating a higher concentration of evolved stars and dust obscuration, and the galaxy is relatively massive. It appears generally undisturbed, without signs of major mergers or tidal features, however there is a slight asymmetry in the upper right. Based on the color indices, the galaxy is relatively luminous, with a moderate star-formation rate. The apparent angular size suggests it is a fairly large galaxy at its given redshift, but this could also be caused by lensing.
