The galaxy presents as a lenticular or edge-on spiral, displaying a smooth, elongated morphology. A central bulge region is visible, appearing slightly more concentrated and yellowish in color than the surrounding disk. The disk itself shows subtle blueish hues suggesting the presence of some star formation, although the overall color profile indicates a population dominated by older stars. The galaxy exhibits a high degree of axial ratio, appearing cigar-shaped. There is no strong evidence of active galactic nuclei activity, significant dust lanes, or major tidal disturbances from this view. The lack of defined spiral arms suggests a relatively passive state, though some slight warping is present in the disk.
