The galaxy presents a generally smooth and concentrated light profile. The core exhibits a yellowish-white hue, suggestive of an older stellar population. There's a gradual fading outward from the center towards the periphery, which is more reddish in color, possibly indicating dust or cooler stars. The overall shape seems elliptical, with the major and minor axes being reasonably close in length, giving it a somewhat rounded appearance. There is no clear evidence of spiral arms or significant star formation regions visible in this image. The galaxy does not appear to be undergoing any major merging events. The morphology is fairly regular with no strong disturbances observed.
