The galaxy appears to be a relatively smooth, elliptical system. Its light profile indicates a centrally concentrated spheroid shape, with a somewhat elongated form. It exhibits a primarily blue hue, possibly indicating ongoing or recent star formation, even if at a low rate. The galaxy is a small size, with no apparent spiral arm structures or other prominent features. The image suggests a galaxy that has largely exhausted its gas supply, resulting in the formation of mostly older stellar populations, but there appears to be a small but noticeable amount of new star formation. There are no strong indicators of any major merger events or tidal disturbances from companions.
