The galaxy presents as a somewhat elliptical structure, elongated along a northeast-southwest axis. A bright, concentrated central bulge dominates the galaxy's luminosity. The bulge exhibits a yellowish hue, suggesting an older stellar population. The surrounding disk is fainter and appears to be relatively smooth, lacking prominent spiral arm structures. The disk shows hints of a bluer color than the bulge, hinting at the presence of younger stars. There are subtle indications of dust lanes within the disk, particularly near the outer edges. Overall, the galaxy appears relatively undisturbed.
