The galaxy presents as an elliptical morphology, displaying a smooth, concentrated distribution of light. The light profile suggests a relatively homogeneous stellar population, lacking distinct spiral arm structures or prominent dust lanes. The object appears highly rounded in shape, with a high degree of central concentration of light. Given the overall red color, we can infer that the dominant stellar population is older, thus resulting in a low rate of star formation. The light distribution is largely undisturbed, with no apparent signs of major merging events or significant tidal interactions.
