The galaxy presents a somewhat elongated, smooth morphology. There is a subtle color gradient across the galaxy body; the bluer light appears dominant towards one end, while the opposite end exhibits a redder hue. Given its overall shape, this could represent a disk galaxy seen at an angle. A more precise classification requires greater image resolution. No signs of active galactic nuclei (AGN) or strong star formation are immediately evident from the color profile. There is no obvious sign of disruption or a major merger event. Its fairly regular shape and color profile suggest a galaxy dominated by older stellar populations.
