The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration with a smooth light profile. The color appears red-shifted, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy exhibits a high degree of rotational symmetry, with no apparent spiral arms or bar structures. The overall structure is relatively undisturbed, showing no signs of recent major mergers or tidal interactions. There might be a slight indication of minor disturbance in the outskirts, but this is highly uncertain given the resolution. The overall form is generally round with a relatively high degree of smoothness.
