The galaxy presents as a single, relatively smooth object. There is evidence of a central bulge, appearing as a bright, concentrated region. A subtle, diffuse disk structure surrounds the bulge. The overall color is a mix of yellowish-white in the center, transitioning to bluish hues in the outer regions of the disk. There are no immediately apparent spiral arm structures. The galaxy exhibits a generally rounded morphology, with only minimal deviations from a circular shape. There are no obvious signs of any major disturbances or ongoing merger activity. Faint irregularities in the outer disk might hint at minor disturbances or interactions, though further observation would be needed to verify this.
