The galaxy presents as a spiral type. There are multiple spiral arms with indications of tight winding, extending from a moderate-sized central bulge. The arms show distinct patchiness, suggesting ongoing star formation regions. The color profile exhibits a gradient with a yellowish hue concentrated in the bulge, transitioning to bluer tones in the outer spiral arms, indicative of varying stellar populations. The overall morphology appears largely undisturbed, with no immediate signs of major merging events, although minor disturbances cannot be ruled out.
