The galaxy presents as a spiral type, viewed at an angle that is approaching face-on but still shows some inclination. Distinct spiral arms are visible, extending outwards from a central bulge. The bulge appears moderately sized, though its exact morphology is difficult to ascertain due to the image resolution. There seems to be no evidence of a strong central bar structure. 

The spiral arms are not uniformly bright, exhibiting variations in luminosity and color, suggesting differing populations of stars and gas along their lengths. This is indicative of active star formation regions within the arms. There appears to be no major merging or tidal disturbance, but some mild asymmetry is present.
