This galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is observed, appearing relatively smooth and rounded. The disk component is characterized by a relatively thin and elongated morphology. There is evidence of structure within the disk, although it is somewhat diffuse in appearance. The galaxy exhibits a color gradient, with the central bulge displaying a yellowish hue, which could indicate an older stellar population, while the disk shows hints of bluer regions, which suggest the presence of younger stars. There is no obvious sign of any major interaction or merging event, but there may be evidence of minor disturbances within the galaxy.
