The galaxy appears as an elongated, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a high density of stars. The color profile transitions from a yellowish-white core to a more bluish hue in the outer regions. This color shift might indicate younger stellar populations in the outer regions, potentially indicating some low levels of star formation activity.  There is a slight asymmetry. While largely smooth in appearance, there appear to be small disturbances from smoothness in the structure, suggesting possible recent interaction.
