This galaxy exhibits a discernible disk structure, though its overall form appears somewhat irregular. The central bulge is prominent and displays a smooth, concentrated light distribution, transitioning into a more diffuse and less structured disk. There is faint suggestion of spiral arms or other features within the disk, with subtle color variations indicating potential regions of star formation, particularly a slight redness within the disk. Overall, the galaxy appears moderately luminous. There is no strong evidence for ongoing major merger activity, but there is a slight irregularity or disturbance within the galaxy's morphology.
