The galaxy presents a largely smooth and rounded morphology. There is a central concentration of luminosity that appears yellowish-white, which could imply an older stellar population dominating the core. Moving outward from the core, the galaxy's light gradually fades, displaying a more diffuse and reddish hue in the outer regions. This color gradient might indicate a radial difference in stellar populations or dust content, with relatively little star formation occurring. There are no obvious spiral arm structures or major disturbances visible in the image. The galaxy appears relatively isolated, with no immediately apparent signs of ongoing merging activity or close companions, though there might be some minor asymmetry hinting at possible past interactions. The overall impression is that of a relatively quiescent, evolved system.
