The galaxy presents as a relatively bright, disk-like structure. Its morphology appears largely smooth, with a central bulge region that exhibits a slightly more concentrated luminosity. The overall shape tends toward elliptical, with an axis ratio indicating it is close to round, as opposed to highly elongated. There's a suggestion of some minor disturbances in the galaxys overall structure, but these are not dominant features. No major merging or tidal tails are apparent. Color gradients indicate the presence of varying stellar populations. The galactic disk exhibits bluer hues, likely due to ongoing star formation.
