The galaxy presents as a relatively smooth, elliptical morphology, with a concentrated central bulge region exhibiting a yellowish hue. There is a slight extension along one axis, deviating from a perfectly spherical shape. The color suggests a population of older stars with minimal ongoing star formation. No distinct spiral arms or dust lanes are discernible. There are some possible very minor disturbances in the outer regions, but they are not clearly defined. The overall structure appears mostly undisturbed, without evidence of major mergers or tidal interactions.
