The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with a high degree of central concentration. The core region shows a yellowish-white hue, potentially indicating an older stellar population. A faint greenish-blue halo surrounds the central region. The outer edges of the galaxy diffuse into the background sky, indicating a lack of distinct boundaries. No obvious spiral arm structures or dust lanes are visible within the galaxy's structure, which further supports its classification as an elliptical type. The overall appearance suggests a relatively quiescent galaxy with little ongoing star formation, although the presence of a faint greenish-blue halo could indicate a small amount of ongoing star formation. There are no signs of major mergers or significant tidal disturbances.
