The galaxy presents as a primarily smooth, elliptical morphology. The core is relatively concentrated with a high degree of luminosity. It appears slightly oblong. A faint halo surrounds the central region. There is some suggestion of a subtle disk-like structure, but this is not a prominent feature. There is no evident ongoing merger activity or significant tidal disturbance. The color profile suggests the presence of an older stellar population, as its concentrated core is relatively red.