The galaxy presents a largely smooth and symmetrical appearance, suggesting an elliptical morphology. The light distribution is concentrated towards the center, with a noticeable decrease in intensity moving outwards. A faint, diffuse halo surrounds the central region. The color is predominantly yellow-orange, potentially indicative of an older stellar population, although some bluer regions are observed in the halo. There is no clear evidence of spiral arms or significant dust lanes. The overall structure implies a relaxed system, without obvious signs of recent major mergers or tidal disturbances.
