The galaxy presents as a spiral with a moderately sized bulge. The spiral arms are well-defined, exhibiting a relatively tight winding pattern and a notable blue hue, suggesting ongoing star formation within the disk. The arms display some patchiness, possibly indicative of HII regions or dust lanes. The bulge appears smooth and yellowish-white, hinting at an older stellar population. The overall shape is elliptical, suggesting the galaxy is viewed at an angle, but not completely edge-on. There's no obvious sign of a strong central bar structure, but a weaker structure is not ruled out. No major signs of disturbance or ongoing merger activity can be seen, although some minor asymmetry can be detected.
