The galaxy presents as a single, albeit complex, luminous object. A distinct, centrally concentrated region exhibits a yellow-orange hue, suggesting a population of older stars. This concentration appears to be interacting with or merging into another similar concentration. No spiral arm structures are discernible. The overall shape appears somewhat rounded, with an extension along one axis, hinting at a possible tidal feature or ongoing merger event. The light is relatively smooth, with a possible distortion in structure to one side, with faint blue scattered light, indicative of a possible star forming region.
