The galaxy appears to be a spiral galaxy, although its orientation is not perfectly face-on. There is evidence of well-defined spiral arms emanating from a central bulge. The bulge is a moderate size in comparison to the rest of the disk, although it does appear prominent, contributing significantly to the overall luminosity of the galaxy. The spiral arms are somewhat flocculent. There appears to be a slight distortion, potentially suggestive of a minor gravitational interaction, though no other galaxy is clearly visible in the immediate vicinity. The dust lanes are somewhat difficult to discern, but they appear to be present, particularly on the near side of the galaxy. The color suggests a moderate level of ongoing star formation. There is no strong central bar feature visible. The disk appears to be the most dominant feature of this galaxy.
