The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The bulge exhibits a yellowish hue, potentially indicating an older stellar population. Surrounding the central bulge is a disk that displays a bluer color, suggesting the presence of younger, hotter stars and regions of ongoing star formation. The disk appears relatively smooth, lacking prominent spiral arm structures, though there seems to be some subtle disk asymmetry on one side. The light distribution suggests it is a relatively massive system. Overall, the galaxy appears relatively undisturbed.
