The galaxy presents as a spiral type, observed at a significant inclination, but not quite edge-on. Two distinct spiral arms are readily discernible emanating from a moderately sized central bulge. These arms appear loosely wound and extend a considerable distance from the galactic center. The galactic disk displays a somewhat patchy structure, indicating regions of active star formation. The overall color suggests a mixed stellar population, with evidence of both older, redder stars and younger, bluer stars, particularly within the spiral arms. There does not seem to be an extreme central bar structure but the center appears elongated or slightly irregular. The galaxy does not show obvious signs of a major merger event, although there is some visual indication of a slight tidal disturbance, perhaps indicating a minor interaction. The bulge component has no visible dust. 
