This galaxy exhibits a flattened, elliptical morphology. The central bulge appears bright and yellowish, possibly indicating an older stellar population with a lower rate of star formation. Moving outward from the core, the color transitions to a bluer hue within the disk, suggesting the presence of younger, hotter stars. The disk shows a smooth texture, but it is still likely that it features subtle spiral arm structures not easily visible in the image. Overall, the galaxy appears relatively undisturbed, without any major signs of ongoing mergers or tidal disruptions, however there may be some minor disturbance. Its elongated shape suggests a significant degree of rotational support.
