The galaxy exhibits a complex morphology. The primary structure appears to be a luminous, centrally concentrated elliptical or lenticular galaxy. It presents a relatively smooth appearance. There is evidence of a potential minor merger event occurring with a smaller, irregular dwarf galaxy. This smaller galaxy shows a bluer color, which may indicate the presence of younger stars and ongoing star formation. There is likely some degree of tidal disturbance present, although the degree is uncertain. The galaxy is likely relatively massive, and appears to have a relatively low star formation rate.
