The galaxy presents as a centrally concentrated, relatively smooth object with a moderately elliptical shape. The core exhibits a yellowish-white hue, possibly indicative of an older stellar population. Surrounding the central region is a faint, diffuse halo that displays a subtle bluish tint. This suggests the presence of a younger, hotter stellar population within the outer regions of the galaxy. There is no clear evidence of spiral arm structures or significant dust lanes. The overall appearance is consistent with that of an early-type galaxy. There seems to be little to no evidence of an ongoing major merger, although minor tidal disturbances cannot be ruled out based on this image alone.
