The galaxy presents as an elliptical morphology, appearing largely smooth and featureless at this resolution. It exhibits a concentrated central bulge, which suggests a higher stellar density towards the galactic core. The colour profile indicates a bias towards redder wavelengths, consistent with an older stellar population and diminished recent star formation. There is no discernible disk structure or spiral arm morphology. Based on its shape, it appears to be somewhere between round and slightly elongated. There is no obvious signs of merging. Overall, the galaxy appears undisturbed.
