The galaxy presents as a somewhat elliptical structure with a smooth, centralized concentration of light. A prominent bulge region is readily apparent, displaying a yellowish hue, indicating an older stellar population. Fainter, more diffuse emission extends outwards, hinting at a possible disk component. A faint bluer glow is observed at the edges, which may suggest more recent, low-level star formation. Overall, the galaxy shows signs of being relatively massive, and appears to have undergone a significant amount of its star formation activity in the past. Morphologically, the galaxy does not appear to be undergoing any major merger events, though there may be some signs of minor interaction or disturbance.
