The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution suggests a higher density of stars towards the core, gradually decreasing outwards. The color profile indicates a relatively homogenous stellar population, with a slight bluer tint in the outer regions and a central yellowish hue. The galaxy lacks any distinct spiral arm structure or significant dust lanes. The overall appearance suggests a relatively evolved system with a low star formation rate. There is no obvious sign of any major merger events, though subtle asymmetries might be present. The round shape indicates little distortion in the overall structure.
