The galaxy presents as a somewhat elliptical, centrally concentrated object. Its core exhibits a yellowish-orange hue, suggesting an older stellar population and potentially a lower rate of ongoing star formation in the nuclear region. The outer regions of the galaxy show a bluer color, possibly indicating the presence of younger, hotter stars. There is some subtle evidence of a disk component. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a faint halo surrounding the galaxy.
