The galaxy presents as a disk galaxy, viewed at a moderate inclination. Its central bulge is prominent and appears to be comprised of older stellar populations, indicated by its yellowish hue. The disk component exhibits a bluer color, suggestive of ongoing or recent star formation, though without clear, defined spiral arm structures. There is a slight asymmetry to the galaxy's overall shape. The galaxy does not appear to be undergoing a major merger, though there could be some minor gravitational disturbance present. The galaxy appears relatively isolated in its field, without any obvious, immediate galactic neighbors suggesting recent tidal interactions.
