The galaxy presents a largely smooth and rounded morphology. There is a dominant central bulge region that appears quite luminous and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population dominating this region. Moving outwards from the central bulge, the galaxy gradually fades in intensity. There's minimal apparent structure indicative of spiral arms or a disk. Faint blue tinges are barely visible, suggesting that there is minimal recent star formation. The object's apparent roundness indicates a system viewed close to face-on, but with a distinct overall spheroidal shape. There are no clear signs of recent or ongoing mergers, such as tidal tails or significant distortions in its overall shape. The galaxy appears relatively isolated within the field.
