The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. Its light profile appears smooth, with no immediately discernible spiral arm structures or prominent dust lanes. The central region exhibits a bright, diffuse glow, transitioning to a fainter, more extended halo. The color gradient suggests a slightly redder hue in the central regions compared to the outer edges, potentially indicating an older stellar population towards the core. There are no obvious signs of a major ongoing merger, though subtle asymmetries or minor disturbances can't be ruled out from this image alone. The galaxy appears relatively isolated. It is a galaxy with ongoing, moderate levels of star formation. The overall appearance suggests an evolved system, with a relatively high degree of symmetry.
