The galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population and/or significant dust obscuration. Moving outward from the core, the galaxy transitions into a fainter, somewhat bluer halo. This suggests a younger stellar population in the outer regions, possibly resulting from ongoing or recent star formation. There appears to be a slight disk-like morphology to the galaxy with some minor disturbances. There is a very small asymmetry in the outer halo. Overall the galaxy is neither a pure elliptical or spiral, and may have some characteristics of both.
