The galaxy presents as an edge-on spiral with a distinct disk structure. A prominent central bulge is observed, appearing brighter and more concentrated than the surrounding disk. The bulge exhibits a smooth, rounded morphology. The disk is relatively thin and elongated, with a slight warp or curvature visible along its length. There is no evidence of significant ongoing mergers or major disturbances in the galaxy's overall structure, although minor irregularities or disturbances cannot be ruled out. The galaxy displays a color gradient, with the central bulge exhibiting a yellowish-orange hue, indicative of an older stellar population, while the outer disk appears slightly bluer, potentially suggesting the presence of younger, hotter stars and ongoing star formation. Overall, the galaxy appears as a relatively isolated and undisturbed spiral galaxy, seen edge-on from our perspective.
