The galaxy presents as an elongated, disk-shaped structure, viewed at a significant edge-on angle. A central bulge is visible, exhibiting a yellowish hue suggesting an older stellar population. The galactic disk appears relatively smooth, with subtle variations in brightness and color. There is a suggestion of some dust lanes within the disk, slightly obscuring the light from stars. The overall morphology indicates that this galaxy is likely a spiral or lenticular type, although the edge-on orientation obscures any spiral arm structure. There appears to be little to no ongoing major merging activity, although there might be some minor disturbances. Based on the colors, it seems to have a small amount of star formation.
