The galaxy presents as a relatively smooth, edge-on spiral. A central bulge is clearly visible and exhibits a yellowish-white hue, suggesting a population of older stars. The disk, viewed nearly edge-on, displays a subtle color gradient, transitioning from the yellowish-white of the bulge to a slightly bluer tint in the outer regions. This implies ongoing star formation within the disk. A dust lane is not easily apparent, though some minor irregularities are visible in the disk structure, suggesting some dust obscuration or minor disturbances. No distinct spiral arms are visible. The overall morphology suggests a galaxy that is not currently undergoing a major merger.
