The galaxy presents as a smooth, concentrated structure with a predominantly elliptical morphology. The central region exhibits a high degree of luminosity, gradually decreasing towards the outer edges. There are no apparent spiral arms or distinct disk features visible. The color profile appears relatively uniform across the galaxy, with a slight shift towards redder wavelengths. No significant tidal disturbances or ongoing merger activity are discernible. The galaxy appears to be relatively isolated, showing no signs of interaction with neighboring galaxies within the immediate field of view.
