The galaxy appears as a single, diffuse object with an elliptical morphology. The light distribution is centrally concentrated and generally smooth, with a possible faint extension or tidal tail on the northern side. There is a distinct color gradient, transitioning from a yellower core region to bluer, fainter outer regions. This may indicate a varying stellar population and age across the galaxy, with an older population toward the center and younger stars in the periphery. The overall structure suggests a relatively evolved system that may have undergone past interactions or minor disturbances. There is also an indication of ongoing merger activity, as the galaxy appears to be gravitationally interacting with a smaller and more compact galaxy.
