The galaxy presents as a moderately elliptical system, exhibiting a smooth, diffuse appearance across its body. There is no discernible spiral structure or prominent dust lanes. The light profile indicates a concentration towards the center, suggesting a dominant bulge component. The galaxy appears to be in the early to mid-stages of a merger with a smaller galaxy, as it has a small component that seems gravitationally bound to it. The system's color is predominantly redder, indicative of an older stellar population.
