The galaxy exhibits an elliptical morphology, with a smooth, centrally concentrated bulge dominating its overall structure. The core displays a bright, luminous glow, suggesting a dense concentration of stars within this region. There is a subtle disk-like component visible, slightly tilted from our line of sight, contributing to the galaxy's flattened appearance. The galaxy appears largely devoid of prominent spiral arms. A slight color gradient is visible, with bluer hues toward the outer regions and redder tones dominating the central bulge, indicating a potential transition in stellar populations, with younger, bluer stars residing further from the center. There's an indication of a slight disturbance in the morphology, perhaps a minor interaction with a smaller system.
