The galaxy presents as a relatively smooth, elliptical structure. The central bulge is prominent, displaying a concentrated luminosity with a yellowish-red hue, suggesting an older stellar population. The outer regions exhibit a gradual decline in brightness, fading into the background sky. The galaxy's overall color is dominated by redder wavelengths, indicative of evolved stars and a lower rate of ongoing star formation. There may be slight hints of a disk structure, though it is not distinct and blends into the spheroid. There are no clearly discernible spiral arms or significant dust lanes. The galaxy appears to be relatively undisturbed, without major signs of tidal interactions or recent merger events. The overall morphology suggests a galaxy transitioning towards a more quiescent state.
