The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There is a lack of discernible spiral arm structure or distinct features, suggesting an older stellar population. The galaxy exhibits a nearly perfect circular shape with no visible tidal disturbances or ongoing merger activity. The color profile appears generally uniform, with a slight reddening towards the central region, indicative of a possible accumulation of older, redder stars in the core. There is a faint, extended halo surrounding the main body of the galaxy. Overall, the galaxy appears to be a well-evolved system.
