This galaxy exhibits a generally smooth morphology, though some features disrupt its overall uniformity. Its color profile suggests a mix of stellar populations, with slightly redder hues dominating. Evidence of possible disk-like structure exists, but is not dominant. There is an irregular feature to the right side, possibly a merging minor companion. Alternatively, this could be a tidal tail or other sign of a minor disturbance. The galaxy's shape is roughly elliptical, but appears slightly perturbed from a perfect ellipsoid. Some evidence suggests possible active or recent star formation. Overall, it appears to be a galaxy undergoing some form of interaction or internal instability.
