The galaxy presents as a centrally concentrated, generally smooth light distribution. The core region is a bright, yellowish-white, suggesting an older stellar population. Moving outwards from the core, the color shifts towards a slightly bluer hue. This might indicate a younger stellar population in the outer regions. The galaxy exhibits a nearly circular morphology, with no obvious signs of spiral arms or a distinct disk structure. There are no clear indications of active galactic nuclei activity or significant dust lanes. The galaxy appears relatively undisturbed, with no prominent tidal features or evidence of a recent major merger event. The faintness of bluer color could indicate an ongoing, but low level of star formation. The size of the galaxy is moderately compact.
