The object is a disk galaxy, observed nearly edge-on. A prominent central bulge is apparent, exhibiting a slight boxy morphology. The disk appears relatively smooth, lacking obvious spiral arm structures. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer disk to a yellow-white color in the bulge, indicating an older stellar population in the central regions. There is no apparent evidence of a major ongoing merger, though there are subtle irregularities that may suggest minor tidal disturbances or accretion events.
