The observed galaxy presents a moderately bright appearance in the optical bands. It appears to be a relatively compact object. The overall morphology suggests a system with some features present; no single central bulge is obvious. Some evidence of disturbance, possibly from a recent interaction or minor merger, is visible. The red and green color index suggests a population of moderately young stars or significant dust reddening. However, some degree of ongoing star formation may be indicated by the brightness in the green filter. There is no evidence of a grand design spiral structure. 
