The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth with a noticeable absence of defined spiral arms or distinct substructures. A bright central bulge is present, which appears somewhat asymmetrical. The primary axis of elongation extends in a roughly horizontal direction across the image. The color profile suggests an aging stellar population with the dominant color being in the redder wavelengths. The galaxy is likely an elliptical type, though a significant disk component cannot be ruled out from visual inspection alone.
