The galaxy presents as an edge-on spiral, displaying a flattened disk morphology. A prominent central bulge is visible, exhibiting a rounded structure. The disk is primarily composed of older stellar populations, inferred from the yellowish hue. Some areas of bluer light indicates regions of more active star formation. There is evidence of some minor tidal disturbances or interactions, as subtle morphological distortions are visible. Overall, the galaxy appears relatively undisturbed, lacking any major merging features.
