The galaxy presents an overall elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated bulge, appearing relatively smooth in texture and yellowish-orange in color, suggesting an older stellar population. This core region transitions outwards into a fainter, less defined disk structure. Subtle color gradients are visible within the disk, with hints of bluer regions intermixed with the prevalent yellow-orange hues, potentially indicating areas of more recent star formation, though these features are not particularly pronounced. There is no evidence of a spiral arm structure or any signs of major disturbances or ongoing merger activity, although there appears to be minor visual irregularity in the outer region of the disk, suggesting a possibility of a minor interaction. The galaxy's overall light profile suggests it is a relatively evolved system.
