The galaxy presents as a largely smooth, elliptical-like structure. There is a concentrated central bulge that is a warm yellow hue, suggesting an older stellar population. Moving outward, a slight disk-like structure can be implied through a marginal flattening. This region shows some color variation, transitioning toward greenish hues which might indicate pockets of star formation, though they do not appear as distinct spiral arms or regions of intense activity. The overall light distribution is fairly smooth with no clear signs of major mergers or significant tidal disturbances, indicating the galaxy is relatively relaxed in its morphological state.
