The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. It appears quite round, showing minimal deviation from circularity. The central region exhibits a bright, concentrated core, suggesting the potential presence of an actively accreting supermassive black hole, though more data would be needed to confirm this. The color profile appears consistent with an older stellar population, indicated by the redder hues observed in the galactic bulge and fainter outer regions. There is no apparent indication of major tidal disturbances or ongoing mergers in this image, although minor perturbations can't be ruled out based on this image alone. While the image is limited, the smooth morphology, and color profile suggest it may be an elliptical galaxy. The galaxy's size appears relatively compact.
