The galaxy presents a relatively smooth morphology, with a somewhat elliptical, rounded shape. There is a hint of a disk-like structure. The color profile suggests a significant population of older stars, indicated by the reddish hue in some regions, but there is also evidence of ongoing or recent star formation, as suggested by the presence of bluer regions within the galaxy. There is no obvious presence of any spiral arm structure. The galaxy does not appear to be undergoing any major merger events. It seems to be a fairly isolated system, with perhaps minor disturbances in its structure.
