The galaxy presents as a disk-shaped system, exhibiting a smooth overall structure with a notable central bulge. The bulge appears to be primarily composed of older stellar populations, indicated by its yellowish hue. The disk shows some defined structure, but lacks prominent spiral arms. A slight bluer tint is observed within the disk region, potentially indicating pockets of more recent star formation activity. The galaxy's elongation suggests it is viewed at a considerable angle relative to its face-on orientation. There is no obvious evidence of strong tidal interactions or major mergers, although a hint of minor disturbance may be present in the outer regions of the disk. The galaxy appears to be a relatively massive system with moderate star formation.
