The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. The core region shows a bright, yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the light gradually diffuses into a bluer halo. This suggests the presence of a more distributed population of younger stars. The overall shape is elongated with an axis ratio significantly deviating from a perfect circle but not extremely oblong, placing it somewhere in between. There is no obvious indication of spiral arms or significant dust lanes. There is a very slight asymmetry, hinting at a potential minor disturbance or interaction with a smaller system. The estimated size suggests that it is a galaxy of moderate size. The color profile implies a moderate amount of star formation for a galaxy of its type and age.
