The galaxy presents as a relatively smooth, elliptical form. It exhibits a dominant central bulge that appears yellowish-orange, suggesting an older stellar population. The galaxy lacks prominent spiral arms. The shape is elongated, more cigar-shaped than spherical. There is evidence of a slight disturbance or irregularity, but no major merger is apparent. It is likely a massive galaxy. The star formation rate appears suppressed, consistent with a population of older stars. The galaxy is a reddish color, which matches the older population and lack of recent star formation.
