The galaxy presents as a disk galaxy, observed at an oblique angle, showing a slight inclination relative to our line of sight. A prominent central bulge is visible, exhibiting a yellowish-red hue, possibly indicating an older stellar population. Fainter, bluer regions appear interspersed within the disk component, suggesting ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a subtle hint of spiral arm structure within the disk, although the resolution limits detailed observation. The disk extends beyond the central bulge, and appears relatively smooth. 
