This galaxy appears to be a spiral galaxy, viewed at an oblique angle, not quite edge-on but significantly tilted relative to our line of sight. The central bulge is a bright, concentrated yellow-orange hue, indicative of an older stellar population. The spiral arms are not well-defined and appear somewhat tightly wound. There is a slight asymmetry in the arm structure. The overall color profile suggests a relatively low star formation rate. Some slight disturbance or irregularity is hinted at, but it is generally a fairly regular structure. The galaxy appears relatively isolated.
