The galaxy presents as a moderately bright, elliptical structure with a smooth, diffuse appearance. The central region is noticeably brighter and exhibits a yellowish-white hue, suggestive of an older stellar population. The outer regions display a more reddish tint, potentially indicating the presence of dust or a population of cooler, redder stars. There is a slight flattening of the galaxy shape, with a ratio of the semi-minor to semi-major axis around 0.8, indicating a deviation from perfect circularity. No distinct spiral arms or significant dust lanes are visible. The galaxy appears relatively undisturbed, showing no major signs of ongoing mergers or tidal interactions. The overall morphology suggests a mature elliptical galaxy with a substantial spheroidal component.
