The galaxy presents as a well-defined elliptical structure with a concentrated central bulge. The core region exhibits a bright, yellowish-orange hue, possibly indicating an older stellar population. The galaxy appears relatively smooth in overall texture, with no prominent spiral arms or disk-like features immediately visible. The shape is somewhat elongated, suggesting a deviation from perfect spherical symmetry. There is a slight hint of bluer light in the outskirts, potentially indicating some minor, recent star formation activity in those regions, although the rate is likely very low. There is no evidence of any major mergers or tidal disturbances and the galaxy is relatively isolated and undisturbed. 
