The galaxy appears to be a disk galaxy, viewed at a high inclination. There is evidence of a central bulge, though it appears small relative to the overall size of the disk. The disk shows hints of spiral structure. The color distribution suggests a mix of stellar populations. There are regions of blue light, suggestive of ongoing star formation, particularly within the disk. The overall shape appears relatively smooth, with no obvious signs of major mergers or strong tidal disturbances. The light distribution is not perfectly uniform, suggesting that star formation and stellar density are not constant throughout the galaxy. The galaxy appears somewhat flattened. The galaxy is estimated to have a mass of approximately 10^10.7 solar masses. It exhibits a relatively low star formation rate.
