The galaxy presents as a spiral, with a moderate inclination relative to the observer. The central bulge is bright and appears yellowish, indicating an older stellar population, which likely contributes significantly to the overall mass. Faint spiral arms extend outwards. The arms show hints of patchy structure, possibly indicating on-going star formation. There is some evidence of a minor disturbance within the spiral arms of this galaxy. The galaxy's form is predominantly in-between a round and cigar shape. There is no strong evidence of a major merger, although there could be a minor interaction occurring.
