The galaxy presents as a luminous, centrally concentrated object. Its overall morphology appears relatively smooth, with a dominant spheroidal component. Color gradients suggest an older stellar population dominating the galaxy's core, trending toward slightly bluer colors in the outskirts. The object's shape appears somewhat elliptical, though it is difficult to precisely assess its axial ratio from this single image. There is evidence of a minor disturbance present, which could suggest tidal interactions with a neighboring object. This may be caused by an ongoing or recent minor merger event. There also appears to be some presence of a disk galaxy, but it is difficult to tell due to its more dominant spheroidal nature.
