The galaxy presents as a centrally concentrated, relatively smooth object with a near-spherical morphology. There's a notable lack of defined spiral arms or a prominent disk structure. The light distribution suggests a dominant bulge component. The galaxy exhibits a yellowish-white color, indicating a stellar population that is likely older and less actively forming stars. Faint, diffuse extensions are visible around the main body, hinting at a possible halo or tidal features, but these are not sharply defined. There's no strong evidence of recent or ongoing major mergers.
