This galaxy appears to be a spiral galaxy viewed at a high inclination, possibly edge-on. There is evidence of a central bulge exhibiting a yellowish hue, suggesting an older stellar population within. The disk of the galaxy shows a bluer color than the bulge. While not clearly resolved, there are some hints of spiral arm structure. There seems to be a notable amount of star formation activity. A visual assessment suggests the galaxy may be experiencing minor disturbances, but appears overall as a relatively isolated, well-defined system.
