The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, spheroidal morphology. Its central region displays a concentrated luminosity, with light graduating into a less bright halo. A slight disclike feature is present. The color profile indicates that the central regions are dominated by older stellar populations, with a shift towards redder wavelengths, while the outer regions are less red. There is no discernible spiral arm structure or dust lanes visible, suggesting a lack of significant recent star formation. The galaxy appears relatively undisturbed, lacking evidence of major mergers or tidal interactions.
