The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light profile appears centrally bright, diminishing radially outwards. The overall shape is fairly round, lacking any obvious distortions or tidal features suggesting recent major merger events. Subtle disturbances cannot be ruled out due to image resolution. The color appears to be relatively uniform, trending towards redder hues. No distinct spiral arm structures or prominent star-forming regions are discernible within the observed optical wavelengths.
