The galaxy presents as a roughly elliptical, centrally concentrated object. The core region exhibits a brighter, more intense luminosity, decreasing radially outwards. The overall color is predominantly a pale blue-white, indicative of a moderate population of younger, hotter stars. There are hints of possible minor disturbances in the outer edges of the galactic disc which could be due to minor gravitational interactions. The galaxy appears to be in a relatively quiescent state, displaying minimal evidence of active star formation in the inner regions. Based on its morphology, it leans towards the smoother end of the galaxy classification spectrum.
