The galaxy appears to be a luminous elliptical type. It exhibits a smooth, centrally concentrated morphology with a radial gradient in surface brightness, the luminosity dropping off steadily from the core. There is no indication of spiral arm structures or a prominent disk component. The galaxy appears highly rounded in shape, and does not show any major disturbances or signs of a merger event. The color profile suggests the presence of a relatively old stellar population, with redder hues dominating the overall color. There is minimal evidence of ongoing or recent star formation based on its color, which is consistent with a passive elliptical galaxy at moderate redshift.
