The galaxy appears to be a relatively smooth, disk-shaped galaxy, possibly an early-type spiral or lenticular, given the lack of prominent spiral arms. There is a brighter, more concentrated central bulge. The galaxy appears slightly elongated. There is a smaller galaxy nearby which may be interacting with it. The color of the galaxy is slightly reddish, suggesting it may be composed of older stars, and has a low rate of star formation. The galaxy has a significant mass, with a notable fraction of galaxies being either smooth or having disks.
