The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is somewhat elongated but predominantly rounded. A brighter, more concentrated central region is apparent, possibly indicative of a dense galactic nucleus. The light distribution fades gradually outwards from the center, exhibiting a diffuse halo. There may be evidence of some minor disturbance or tidal interaction present, possibly with a smaller dwarf galaxy. The primary body displays a subtle color gradient, with a slightly bluer hue toward the outer edges.
