The observed galaxy presents as an edge-on spiral, exhibiting a prominent, centrally concentrated bulge. The bulge displays a notably smooth, rounded morphology. A faint disk extends outwards from the bulge, appearing relatively thin and elongated. There is a subtle color gradient observed within the galaxy, with the bulge exhibiting a redder hue, suggesting an older stellar population, while the disk presents bluer tones, indicative of ongoing star formation. No major disturbances or merging features are readily apparent.
