The galaxy presents as an edge-on spiral, or possibly lenticular, system. A prominent, somewhat boxy bulge dominates the central region, exhibiting a yellowish-white hue suggestive of an older stellar population. The disk appears relatively smooth and featureless, lacking distinct spiral arm structures or prominent dust lanes. The disk displays a bluer tint compared to the bulge, hinting at the presence of younger, bluer stars in the disk component. The galaxy shows no visual signs of a major ongoing merger, although some minor asymmetry or disturbance cannot be ruled out based on the available image. Overall, the galaxy appears to be a relatively quiescent system, likely with a low star formation rate.
