The galaxy presents as a largely amorphous structure with a fairly elliptical, almost circular, shape. The light distribution within the galaxy appears smooth and centrally concentrated with no obvious spiral arms or significant disk-like structure. There is a faint, slightly irregular glow emanating from the galaxy's main body, with no distinct features such as prominent dust lanes or star-forming regions visible. The light tapers gradually towards the galaxy's edge. The core is slightly brighter than its peripheral regions. There is no evidence of a recent major merger, but there may be some minor disturbance or interaction present.
