The galaxy presents as a generally smooth, elliptical-like structure with a bright, concentrated central bulge. There is a slight elongation or flattening, but it appears nearly circular. The core region emits strong luminosity, suggesting a high concentration of stars and potentially an active galactic nucleus. Color gradients suggest variations in stellar populations; the central region appears more yellow/white, transitioning to bluer hues in the outer regions. This suggests older stellar populations are concentrated in the center, with younger, bluer stars more prevalent in the galactic disk. A faint, arm-like structure extends to the lower left of the central bulge.
