The galaxy presents a generally elliptical morphology, exhibiting a smooth light distribution without apparent spiral arms or distinct features. The central region displays a brighter, concentrated core, likely indicative of a substantial galactic nucleus. The color gradient transitions from a yellowish core to a reddish hue at the outer edges, which suggests an older stellar population in the periphery. Subtle asymmetries are visible, suggesting potential minor gravitational interactions or disturbances, but there is no clear evidence of a major merger event. The galaxy appears to be of moderate size and mass for a galaxy at its redshift. Based on its colors, there is likely ongoing but low star formation. 
