The galaxy appears to be an elongated, possibly lenticular or edge-on spiral galaxy. There is a smooth, centrally concentrated bulge that exhibits a yellow-orange hue, indicative of an older stellar population. Extending outward from the bulge is a fainter, bluish disk. The lack of distinct spiral arm structures suggests that any spiral arms are either tightly wound, or very faint. There are no signs of any major mergers, tidal tails or streams. The galaxy appears largely undisturbed, but may be experiencing minor interactions as there is a slight warp in the disk. Overall, the galaxy is quite luminous.
