The galaxy presents as a relatively smooth, centrally concentrated object. It displays a yellowish hue at its core, suggesting an older stellar population dominates the central regions. The galaxy appears elliptical in shape, with a slight elongation. There is evidence of a fainter, bluer, disk component surrounding the bulge. There are hints of minor disturbances. The galaxy is not perfectly symmetrical; one side has a more extended and diffuse profile than the other. The overall color indicates moderate levels of ongoing star formation.
