The galaxy appears to be an edge-on spiral, likely at a redshift of approximately 0.067. The central bulge is prominent and appears relatively smooth and somewhat boxy. The disk is elongated, and the dust lane bisecting the galaxy is not clearly visible. There may be evidence of faint spiral arms within the disk, but the resolution limits the ability to definitively confirm the spiral structure. The color distribution suggests an older stellar population overall, with a more pronounced concentration of older stars within the bulge. There is no obvious sign of any major ongoing merger or significant tidal disturbances.
