The galaxy presents a generally elliptical morphology, with a smooth appearance. The central region exhibits a higher surface brightness, appearing more luminous. A subtle color gradient is observed, transitioning from a slightly redder core to a subtly bluer outer region. No distinct spiral arm structure or significant dust lanes are discernible, but some minor disturbances may be present, giving it a slightly irregular form. Overall, the galaxy appears to be of substantial mass, with moderate levels of star formation.
