The galaxy presents as a single, concentrated body with a generally smooth morphology. The central region exhibits a pronounced, bright yellowish-orange hue which gradually fades into greenish tones in the galaxy's outer reaches. There is no evidence of spiral arm structure or a prominent disk within the resolution of the image. The shape appears somewhat elliptical, though tending toward a more rounded appearance. The overall structure suggests a system that is either an elliptical galaxy or a spiral galaxy seen nearly face-on without significant resolved features. There are hints of some minor disturbances, perhaps suggestive of a past or ongoing interaction, but no clear tidal tails or other indications of major merging activity are discernible. The relatively smooth light distribution and color gradients point to a potentially evolved stellar population. The color information suggests that the galaxy is actively forming stars, albeit at a modest rate.
