The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape approximates a circular or slightly elliptical morphology. There is a suggestion of a slight deviation from perfect roundness, but no prominent bar or spiral arms are discernible. The light distribution appears to be mostly uniform, with a gradual decrease in intensity from the center outwards. The core region exhibits a slightly brighter, more condensed appearance. Faint, diffuse features may be present, suggesting potential interactions or minor disturbances, but these are not sharply defined. The galaxy presents a predominantly quiescent appearance based on the limited data.
