This galaxy presents as a flattened, disk-like structure, viewed at a near edge-on orientation. The central region exhibits a concentrated luminosity, indicating the presence of a bulge, likely composed of older stellar populations, exhibiting a yellowish hue. The galaxy's disk shows a subtle blue tint along its edges, which may indicate ongoing star formation within the spiral arms, though distinct spiral structures are not clearly resolved in this image. There is slight asymmetry in the outer regions of the disk, which could be evidence of past interaction or a minor disturbance in the gravitational field. The overall light profile suggests a relatively smooth distribution of stars. No prominent dust lanes are clearly visible.
