The galaxy presents as an object with a relatively smooth morphology. There appears to be a dominant central bulge exhibiting a yellowish-red hue, suggesting an older stellar population concentrated at the galactic center. The outer regions of the galaxy display a bluer color, hinting at the presence of younger stars and possibly some ongoing star formation. The overall shape is close to round. There are no obvious signs of a major ongoing merger, but subtle asymmetries or minor disturbances can not be ruled out. The galaxy appears to be of intermediate size, displaying characteristics of a disk galaxy without highly defined spiral arms.
