The galaxy presents an elliptical morphology, with a smooth light profile across the majority of its body. The galaxy appears to be undergoing a merging event, with multiple apparent nuclei or bright concentrations of light visible within the central region. There are no obvious spiral arm structures. The primary light distribution is concentrated towards the center, fading out towards the edges. The overall color suggests an older stellar population, as indicated by the orange-red hue. There appears to be a tidal tail or minor disturbance to the north. There are no apparent dust lanes within the galaxy.