The galaxy exhibits an elliptical morphology, appearing largely smooth and spheroidal in shape. There is a discernible concentration of luminosity towards the central region, suggesting a prominent galactic nucleus. The overall color profile tends towards the redder end of the spectrum, indicative of an older stellar population and potentially lower levels of ongoing star formation. No distinct spiral arm structure or significant dust lane features are apparent. The galaxy appears relatively undisturbed, with no obvious signs of recent or ongoing merger activity or tidal distortions.
