The galaxy presents a largely smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual falloff in surface brightness towards the edges. There is little to no discernible spiral arm structure or prominent dust lanes. Its color suggests an older stellar population, tending toward redder hues in the optical bands. The galaxy is moderately luminous. There is no obvious indication of a major ongoing merger event, though the potential for minor tidal disturbances cannot be completely ruled out based on the image alone. It exhibits a slight elongation, deviating from a perfectly circular shape.
