The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a bright, concentrated central bulge, suggesting a high density of older stars. The color gradient indicates a yellow or golden hue near the core, which then fades to a dimmer redder color around the edges of the galaxy. This color profile implies an older stellar population, a relatively low rate of current star formation and little dust obscuration. There is some evidence of faint diffuse light surrounding the central region, potentially indicating a halo of stars. No distinct spiral arm structures or strong dust lanes are apparent.
