The galaxy presents as a somewhat smooth, centrally concentrated object with a moderate amount of disturbance visible. Its overall shape approximates a rounded form, though it deviates from a perfect circle. The color profile suggests the presence of intermediate-age stellar populations, showing a notable signal in the g, r, and z bands. The presence of significant disturbances hints at potential ongoing or recent interaction with another galaxy, likely in the form of a merger, given the scale of the disturbance. Star formation appears to be active, as indicated by the galaxy's luminosity. The estimated size is consistent with an average galaxy at its redshift.