The galaxy presents as a disk-shaped system, viewed at a near edge-on angle. A distinct central bulge is observed, appearing smooth and concentrated, exhibiting a yellowish-orange hue. The disk component displays a bluer color profile, suggestive of ongoing star formation activity, which is notably more subdued. The disk appears relatively smooth, lacking prominent spiral arm structures or significant dust lanes. Overall, the galaxy exhibits a generally undisturbed morphology, with no obvious signs of major merging events or tidal distortions. It appears relatively compact, with a high degree of central concentration.
