The galaxy presents as a spiral type, observed at an oblique angle. The central bulge is moderately prominent and exhibits a yellow-white color, indicative of an older stellar population. Spiral arms are clearly visible, displaying a distinct blue hue, suggesting ongoing star formation. The arms are primarily composed of two major branches exhibiting a tightly wound morphology in some areas and medium winding in others, and some loose winding as well. A faint, elongated feature suggesting a bar structure can be discerned bisecting the central bulge. There appears to be some minor asymmetry or disturbance in the outer disk region, although no major companion or tidal tails are clearly apparent. Overall, the galaxy seems to be relatively undisturbed, with a regular spiral structure, although there are faint hints of interaction.
