The galaxy presents as a generally smooth, elliptical object. It exhibits a high degree of circularity in its overall form. The light profile shows a concentrated central region with a gradual decline in surface brightness moving outwards. The galaxy's core appears bright and has a yellow-orange hue, suggesting an older stellar population. There are no obvious signs of spiral arm structures, significant dust lanes, or ongoing major merging activity. Minor disturbances cannot be ruled out, though. It is likely a massive, quiescent galaxy with relatively low specific star formation rate.
