The galaxy presents an elliptical morphology, appearing smooth and relatively featureless. The light distribution suggests a centrally concentrated structure with a gradual decrease in brightness outwards. The isophotes appear elongated, exhibiting a moderate degree of ellipticity. There is no discernible evidence of spiral arms or a prominent dust lane. The color appears generally uniform across the galaxy, with a slightly bluer hue towards the central region, potentially indicating a population of younger stars in the core. The galaxy's overall appearance suggests a relatively evolved system with a modest rate of on-going star formation. There is a subtle indication of minor asymmetry or tidal disturbance.
