The galaxy presents as a diffuse object, exhibiting a generally smooth morphology. There appear to be two prominent, centrally concentrated regions of increased luminosity, suggesting a possible dual core. The overall color appears reddish-yellow, with a slight gradient, likely indicating an older stellar population. The object is estimated to be of substantial size, likely possessing a significant stellar mass. Indications point to ongoing or recent merger activity. While a clear spiral or elliptical structure is not directly discernible, the overall characteristics lead to the classification as a possible early-type galaxy undergoing interaction.
