The galaxy presents as a slightly inclined spiral with a prominent bar structure spanning a significant fraction of its length. The spiral arms are somewhat flocculent, with hints of star formation regions visible as bluer knots within the arms. A notable central bulge is present but does not dominate the overall structure of the galaxy. There is no strong evidence of recent major merger activity, though some minor disturbances in the disk may be present. The galaxy exhibits a relatively smooth appearance overall, with a moderate level of ongoing star formation. The colors are consistent with a mix of stellar populations, with the blue indicative of younger stars and the redder colors suggesting older populations.
