The galaxy presents as an elliptical system, elongated in shape. It exhibits a smooth morphology with no apparent spiral arm structures or prominent dust lanes. The central region of the galaxy appears brighter and more concentrated, suggesting a higher density of stars towards the galactic nucleus. A slight color gradient is observed, with the central regions appearing more yellowish, and the outer regions exhibiting a bluer hue, hinting at potential variations in stellar population. The galaxy does not appear to be strongly interacting with any neighboring galaxies, although there is a possibility of minor disturbances given the presence of a faint, extended halo. No clear evidence of active galactic nuclei activity is readily apparent. The galaxy is observed to be at an approximate distance where its estimated diameter would be around 13 kpc.
