The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape appears to be relatively elliptical, verging on spheroidal. The light profile suggests minimal disc structure, with the majority of the luminosity emanating from the central bulge region. There are possible disturbances in the surrounding stellar halo, indicative of past or ongoing minor interactions. Based on the color profile, blue light is more prominent near the core indicating it is a location of star formation.
