The galaxy presents an elliptical morphology, exhibiting a relatively smooth and diffuse structure. The light distribution is centrally concentrated, gradually decreasing in intensity outwards from the core. There are no prominent spiral arms or a well-defined disk visible. The color profile suggests a predominantly older stellar population, with a lack of significant blue light indicative of recent star formation. The galaxy appears undisturbed, with no signs of tidal features or ongoing mergers, though some minor disturbances cannot be ruled out. The overall impression is that of a mature, passively evolving system.
