The galaxy presents a generally smooth morphology, with a concentrated central region. The light distribution suggests a mostly elliptical shape, though it is difficult to precisely ascertain the ellipticity. The galaxy exhibits a radial color gradient, transitioning from a redder core to bluer outer regions. This may indicate a change in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars in the surrounding areas. There is no strong evidence of spiral arm structure or a prominent disk, which suggests it could be an elliptical or lenticular type galaxy. There do not appear to be any signs of a major merger event. Close inspection does not indicate the presence of prominent dust lanes or strong tidal features. The overall appearance is consistent with a massive galaxy undergoing a moderate amount of star formation.
