The galaxy presents as a largely homogenous structure with a smooth overall appearance. It exhibits a generally round morphology, with a slight deviation toward an intermediate shape. The central region appears brighter than the outer edges, suggesting a concentration of stellar populations towards the core. There's a hint of minor disturbances in the galaxy's structure, possibly indicating past interactions or internal dynamic processes. The light distribution is fairly even across the galaxy, although slight color variations can be seen that might point to differences in stellar population age or composition within the galaxy.
