The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. The galaxy exhibits a relatively smooth appearance overall. A faint disk is visible, oriented roughly edge-on relative to our line of sight. There are no prominent spiral arms apparent. There are only some very slight disturbances, not enough to be considered signs of a major merger, but maybe a minor one. The overall color suggests a relatively evolved stellar population, leaning towards older stars, with a subdued level of ongoing star formation.
