The galaxy appears as a somewhat elongated, lenticular or early-type spiral form, displaying a smooth, diffused light profile with little discernible internal structure. There is a concentration of light towards the center. The galaxy appears to be relatively isolated with no other obvious bright companions. The light distribution suggests a spheroid-dominated system. Faint extensions or tidal features cannot be ruled out, although these are not immediately apparent. The galaxy possesses a slight blue hue suggesting the existence of some young stars or a population with moderately recent star formation activity.
