The galaxy presents as a relatively smooth, elongated structure. It appears to be a disk galaxy, as some disk features are present within the galaxy. The color is slightly bluer in the center than on the edges. While there is a concentration of light in the central region, no prominent, well-defined nucleus is visible. Some evidence of recent or ongoing star formation exists, as hinted by the slight blue hue. The disk appears relatively undisturbed, and there is no obvious sign of an ongoing major merger. There may be signs of a minor disturbance or small companion. The overall impression is of a galaxy with a moderate mass, exhibiting a relatively low star-formation rate.
