The galaxy appears to be a relatively bright, distant object with a generally smooth morphology. It presents a somewhat elliptical shape, tending towards round, with little discernible internal structure visible at this resolution. The galaxy exhibits a color profile slightly shifted toward the redder end of the spectrum. There appears to be some ongoing or recent interaction or merging activity present, influencing the overall morphology and potentially contributing to elevated star formation. There is a slight distortion in the galaxys smooth, rounded shape which indicates it is likely in the process of merging with another galaxy.
