The galaxy presents as a luminous, centrally concentrated object, elliptical in form. It displays a smooth, largely featureless structure, with a gradual decline in brightness from the core outwards. The core region exhibits a distinct yellowish-white hue, indicating an older stellar population. Progressing outwards, the galactic disk appears to incorporate a wider range of colors with some faint bluish tints in the outer edges. The galaxy shows some slight morphological disturbance, potentially the influence of minor gravitational interaction. There does not appear to be a defined spiral structure or strong star forming regions. 
