The galaxy presents as a spiral type, viewed at an angle significantly off from face-on. The spiral arms are fairly well-defined and numerous, but are tightly wound around the central bulge. The bulge appears of moderate size relative to the disk, with a yellowish hue, suggesting an older stellar population within. The disk itself exhibits a bluish tint, indicative of ongoing star formation. There is no obvious bar structure visible. The overall morphology appears relatively undisturbed, with no major signs of recent merging activity or tidal distortions. The system shows some signs of star formation, with the spiral arms showing distinct features, but nothing exceptional.