The galaxy appears to be a spiral, viewed at a high inclination. A prominent central bulge is observed, exhibiting a yellowish-white hue, likely indicative of an older stellar population. The disk appears relatively smooth. The spiral arms are tightly wound. The galaxy's overall shape is elongated, suggesting a classification ranging between an intermediate spiral and an elliptical galaxy. There is no strong evidence of an ongoing major merger, although there is slight asymmetry in the galaxy's morphology.
