The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. The light distribution suggests it's mostly round, though perhaps slightly elongated. The galaxy shows a color gradient, with the central region appearing more yellowish, suggesting an older stellar population. The outer regions of the galaxy exhibit a bluer hue, potentially indicating the presence of younger, hotter stars, but may also be an artifact. There is no evidence of a spiral structure, bar, or significant dust lanes within the galaxy's visible structure. There is no apparent interaction or merging event occurring. Overall, it seems to be a relatively undisturbed system.
