The galaxy presents a smooth, elliptical morphology with a centrally concentrated bulge. There is a noticeable radial gradient in color, transitioning from a slightly bluer core to redder outer regions. No distinct spiral arm structures are observed. The light distribution appears fairly uniform, lacking pronounced features such as dust lanes or star-forming knots. There is evidence of a slight flattening, suggesting a deviation from a perfectly spherical shape. Overall, the galaxy appears consistent with a relatively quiescent, evolved stellar population.
