The galaxy presents as a luminous, centrally concentrated object with a generally smooth morphology. The color profile suggests an older stellar population, with a yellowish hue dominating the core region. There is a slight elongation of the isophotes, deviating marginally from a perfectly circular shape. No distinct spiral arm structure or prominent dust lanes are visible, implying that the galaxy is likely elliptical in nature or a lenticular galaxy viewed face-on. There is a slight indication of possible minor disturbance, such as a plume or tidal tail, but that is unclear.
