The galaxy presents as a moderately luminous, well-defined elliptical system. The light profile appears smooth and centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. There are no apparent spiral arms or prominent dust lanes visible, further suggesting an elliptical morphology. The galaxy exhibits a slightly elongated shape, deviating marginally from perfect circularity. No major disturbances or signs of ongoing mergers are readily apparent in the image, though some minor irregularity in the outer regions cannot be ruled out at this resolution. The color appears generally uniform across the galaxy, with a subtle shift towards redder hues in the central region.
