The galaxy presents as a relatively small, lenticular-like structure with a high degree of smoothness. Its ellipticity suggests it is an elongated disk viewed at an oblique angle. The color distribution appears fairly uniform across the body of the galaxy, showing a relatively homogeneous stellar population with a slight blue hue. There is a subtle concentration of light towards the galaxy's center, indicating the presence of a central bulge. While some faint irregularities are present, they do not suggest any significant tidal disturbances or ongoing major merging events. Overall, the galaxy appears to be a fairly evolved and undisturbed system.
