The galaxy presents an elliptical morphology, appearing somewhat elongated rather than perfectly spherical. A bright, concentrated central bulge is evident. The outer regions of the galaxy exhibit a smoother, more diffuse distribution of light, fading gradually into the background. There is no clear evidence of spiral arm structure or significant dust lanes. The light distribution suggests a relatively evolved stellar population, and the colour profile indicates the presence of older, redder stars. The overall impression is that of a mature, quiescent galaxy, likely with a high stellar mass, undergoing relatively low levels of star formation.
