The galaxy presents a somewhat elliptical morphology. It displays a central bulge region that exhibits a yellowish-orange hue, suggestive of an older stellar population. There appears to be a flattened disk component, though its structure is not sharply defined, possibly due to the galaxy's distance. The disk shows hints of bluer regions, potentially indicative of more recent star formation. While no strong spiral arm structures are visible, there are subtle irregularities in the disk's light distribution that might point to minor disturbances, possibly resulting from a previous interaction. The overall appearance suggests a galaxy that may be in a transition phase, moving from a more actively star-forming state to a more quiescent one.
