The galaxy presents a predominantly smooth morphology. There is a slight suggestion of a disk structure, though the overall form appears largely spheroidal. The color profile indicates an aging stellar population, particularly concentrated within the central bulge, signified by its yellowish hue. There's evidence of ongoing star formation in the outer regions, contributing to a bluer tint. There isn't any clear evidence of a major merger or significant tidal disruption, and the object appears relatively isolated. The structure seems relaxed, suggesting a lack of recent major disturbances.
