The galaxy presents a smooth, elliptical morphology. Its central region exhibits a high concentration of light, appearing nearly uniform in color and brightness. Moving outward from the center, the light gradually diminishes, transitioning to a fainter, less defined halo. The overall color profile appears reddish, suggesting an older stellar population. There is no evident spiral structure or significant dust lane obscuration. The galaxy appears to be relatively isolated, with no clear signs of tidal interactions or nearby companions disrupting its structure.
