The galaxy exhibits an irregular morphology. A dominant, relatively smooth central component displays a yellowish hue, suggestive of an older stellar population. Emanating from this central region is a fainter, more diffuse extension, exhibiting a slightly bluer color. The structure shows signs of disturbance, potentially indicating an ongoing or recent merger event. The primary body of the galaxy appears somewhat rounded. There is evidence of ongoing interaction or tidal features, suggesting it could be in the late stages of a merger. Overall, the galaxy's appearance indicates a system with a significant spheroidal component and morphological features suggestive of interaction. The galaxy shows relatively low star formation.
