The galaxy presents a relatively smooth and somewhat flattened elliptical morphology. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a higher stellar density towards the core. There's a subtle color gradient noticeable, shifting towards slightly bluer hues in the outer regions of the disk, indicating the possibility of ongoing or recent star formation activity in those areas. However, the overall color distribution is dominated by older stellar populations.

The disk is relatively well-defined, and appears mostly undisturbed. The low luminosity of the galaxy indicates the the galaxy is of a moderate mass. The relatively low levels of recent star formation also suggest a relatively low star formation rate.
