The galaxy appears as a large, relatively smooth elliptical or lenticular system. It exhibits a concentrated central bulge that dominates the overall structure, with a gradually decreasing surface brightness moving outwards. The color of the central region is yellowish-orange, suggesting an older stellar population and a lack of significant recent star formation. The outer regions have a slightly bluer tint, hinting at the presence of some younger stars, though the overall star formation rate seems low. The galaxy’s shape is generally elliptical, with a moderate ellipticity, deviating somewhat from a perfect circle. There are no readily apparent spiral arms or strong dust lanes visible, indicating it's likely a more evolved system. There are some minor disturbances detectable, as the system might be interacting or have merged with another in the past. Overall, the galaxy presents as a mature, massive system with a largely quiescent stellar population.
