The galaxy presents as a spiral type, exhibiting a notable central bulge that appears moderately bright and concentrated. The spiral arms are well-defined, displaying a tightly wound morphology. The galaxy has a generally blue hue, suggesting the presence of a substantial population of young, hot stars and ongoing star formation. No bar structure is clearly visible. The disk appears relatively undisturbed, with no major signs of recent merger activity, although there is some minor distortion visible, particularly at the ends of the spiral arms. The isophotes are elliptical, and the galaxy has a substantial angular size.
