This galaxy appears to be a disk galaxy, viewed nearly edge-on. A prominent bulge is visible, exhibiting a rounded shape. The dust lane is prominent. There is little evidence of a spiral arm structure. There appears to be no signs of an ongoing major merger, although minor tidal disturbances cannot be ruled out. The galaxy displays a color gradient, transitioning from a bluer hue at the outer edges of the disk to a redder hue in the central bulge. The color of the bulge suggests an older stellar population. The overall shape is relatively smooth, indicative of a settled morphology. There is some visible star formation.