The galaxy presents as a somewhat elongated structure, likely a spiral galaxy viewed at a high inclination. The central bulge appears prominent and exhibits a yellowish-white color, possibly indicating an older stellar population. The spiral arms are faintly visible, displaying a bluish hue which suggests the presence of younger, hotter stars and ongoing star formation. There is evidence of some disturbances or asymmetries in the disk, although the galaxy is most likely not undergoing any major merging event. The galaxy is likely undergoing relatively little star formation. The galaxy's overall morphology suggests it is neither a pure elliptical nor a grand design spiral, but something in between.
