The galaxy presents a somewhat ambiguous morphology, appearing to be in the late stages of a major merger or collision. The central region exhibits a high degree of smoothing, with a concentrated luminosity. The outer regions of the galaxy show faint, distorted features, possibly tidal tails or disrupted spiral arms, which indicates an interaction with another galaxy. The color gradient suggests the presence of older stellar populations. The galaxy's overall shape deviates significantly from a regular elliptical or spiral, presenting an irregular profile. The distribution of light and color is uneven, supporting the hypothesis of ongoing or recent gravitational interactions.
