The galaxy appears as a moderately luminous, slightly elongated system. The central region exhibits a smooth, concentrated light profile, suggestive of a bulge component. Fainter, more diffuse light extends outwards from the central region, indicating a possible disk or extended halo. There's a hint of a spiral structure, but it is not well-defined and may be flocculent. The color is primarily bluish-white, with the central regions trending towards a more yellow-white hue, possibly indicating an older stellar population concentration. There are suggestions of some disturbances in the outer structure, possibly indicating a past or ongoing minor interaction or merger event. Based on the morphology, this system could be classified as a late-type spiral or an interacting galaxy.
