The galaxy presents as a somewhat smooth, centrally concentrated object, with an apparent spheroid shape. There is a slight elongation, but overall, it leans toward a rounder morphology. A distinct color gradient is observed, with a yellowish-white core transitioning to a reddish hue towards the edges of what is likely a bulge component. There is an orange distinct feature to the upper left, but it appears to be inside of the galaxy. The lack of well-defined spiral arms or strong dust lanes suggests it is either an elliptical galaxy or a spiral galaxy seen at a considerable distance where finer structural details are blurred. The reddish color on the outskirts may be indicative of an older stellar population, whereas the yellower center could imply ongoing star formation, though this is uncertain given the resolution of the image. There is no obvious evidence of ongoing major merging events, although there appears to be minor distortions, such as the orange feature, which suggest possible interactions. Overall, the galaxy appears to be a moderately massive system, possibly an early-type spiral or an elliptical galaxy undergoing passive evolution.
