The galaxy appears as a diffuse, extended object with a relatively low surface brightness. It exhibits a generally smooth morphology, with no immediately obvious spiral arms or bar structures. The color distribution suggests a predominantly older stellar population, with a redder overall hue, although there are subtle variations hinting at potentially younger, bluer regions within the galaxy. There is some suggestion of tidal interactions or morphological disturbance. Further investigation is needed to determine if these are real physical features of the galaxy. Overall, it appears as an elliptical or lenticular galaxy.
