The galaxy appears to be a spiral galaxy, viewed at a significant angle. The central bulge is slightly elongated, and shows a yellowish hue. A disk structure is apparent, exhibiting a bluer color, indicative of ongoing star formation. There appears to be only slight irregularities in the disk, meaning that there could have been a recent minor interaction or disturbance. It does not appear to be undergoing a major merger, as the disk is still relatively intact. The smooth central concentration of light suggests a moderate stellar mass. Based on the color, and disk smoothness, the star formation rate is fairly low.