The galaxy presents as a roughly elliptical object, exhibiting a significant degree of smoothness in its overall light distribution. The central region displays a marked concentration of luminosity, suggestive of a prominent galactic bulge or core. The main body is slightly elongated, transitioning between a rounded and cigar-like shape, where the axis ratio is nearly 1:1 but with some visible deviation. Evidence of disturbances or interactions are present, as the overall structure shows signs of irregularity, potentially hinting at minor or major disturbances due to ongoing or past mergers. There is no single obvious merging event, but the disturbance suggests the possibility of a recent interaction. The galaxy does not display prominent spiral arms or other features commonly associated with disk galaxies, and overall the image does not reveal substantial amounts of resolved fine structure.
