The galaxy presents as a somewhat elliptical structure, displaying a smooth, diffuse morphology overall. Its core exhibits a concentrated luminosity, shifting towards yellower wavelengths, suggesting an older stellar population in the central region. The outer regions, while less luminous, show bluer tints, potentially indicative of younger stars or ongoing star formation. While the galaxy generally appears as a singular object, there's subtle irregularity in its form, with a slight elongation along one axis. Despite the dominant smooth appearance, there are hints of subtle features or disturbances in the outskirts. The colours suggest that there are signs of recent star formation occurring, at very low levels.
