The observed galaxy presents a predominantly smooth morphology with an elliptical or spheroidal shape. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There's little evidence of spiral arms or a prominent disk-like structure. The galaxy exhibits a relatively uniform color gradient with slight color differences. The overall structure seems undisturbed, indicating that no major mergers are visibly distorting its shape. There may be minor irregularities, but these are not significant enough to indicate substantial tidal interactions.
