The galaxy presents as a somewhat smooth, elliptical form, exhibiting a concentrated central bulge that graduates outwards into a more diffuse halo. The light distribution indicates a centrally bright core. The galaxy's color appears to be relatively uniform across the structure, with subtle variations potentially indicating differences in stellar populations or dust content, and it appears more reddish in color. The overall structure suggests a system in a relatively evolved state. There is potential indication of some morphological disturbance or minor interaction.
