The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution indicates a near-spherical shape, lacking prominent features like spiral arms or a distinct disk. Color gradients suggest a potentially older stellar population dominating the central region, indicated by the yellow hue. There may be hints of ongoing or recent star formation evidenced by tinges of bluer colors. There is no distinct bar or ring structure. The galaxy does not appear to be undergoing a major merger or significant tidal disruption. Minor asymmetry is present in the shape, hinting at a potentially interacting with a nearby companion. 
