The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is little indication of prominent spiral arms or significant dust lanes. The overall color profile suggests an older stellar population, with a yellow-white hue dominating the central region, transitioning to a slightly redder color in the outer regions. This is consistent with a lower rate of star formation. It has a roughly round morphology and does not appear to be undergoing any major mergers or disturbances. The light is relatively evenly distributed, with a gradual decrease in brightness as you move from the core to the outer edges, further supporting the classification of a smooth galaxy.
