The galaxy appears as a centrally concentrated object, approximately elliptical in shape. The core is bright and intensely luminous, exhibiting a yellow-white hue indicative of an older stellar population. The luminosity decreases radially from the core. A faint disk or halo is suggested at the periphery. There are no prominent spiral arms, bar structures, or dust lanes visible. The overall color suggests a relatively low rate of ongoing star formation. The lack of significant asymmetry suggests the galaxy is relatively undisturbed, showing no major signs of recent merger activity.
