The galaxy presents as a centrally concentrated system with a smooth, diffuse morphology. Its color profile suggests an older stellar population, potentially with a dominant population of evolved stars. The galaxy appears elliptical or spheroidal in shape, lacking any readily discernible spiral arm structure or prominent dust lanes. The system appears relatively isolated, with a hint of minor gravitational interaction affecting the morphology. There is a neighboring galaxy that might have some tidal interactions that do not seem very violent.&#x20;
