This galaxy presents as a relatively compact object with a somewhat smooth appearance in this image. It exhibits a predominantly round morphology, although with some slight deviation from perfect circularity. There is a hint of some internal structure, possibly indicating either a disk-like feature or some form of interaction. The color suggests a redder overall population of stars, with minimal evidence of active star formation regions. There is a potential sign of minor disturbance, though any ongoing merger activity appears to be insignificant or past it's peak.