The galaxy presents as a relatively smooth, elongated structure. The color profile exhibits a clear gradient, transitioning from bluer tones at one end to redder hues at the opposing end. One region shows hints of disk-like morphology, while the other is notably redder and elongated, suggestive of a spheroidal component. Overall, the galaxy presents a moderate to high luminosity, with a mass on the higher end. This galaxy may be undergoing some merging, and there is a significant amount of star formation occurring within the galaxy.
