The galaxy presents as a centrally concentrated spheroid, appearing largely smooth in overall texture. Its color profile suggests a dominant older stellar population, exhibiting a reddish-yellow hue at the core which fades slightly into a greenish color at the edges. The morphology indicates an elliptical galaxy, lacking any apparent spiral arm structure or prominent dust lanes. Its overall shape is generally round, with only minimal deviations from circular symmetry. There is no clear evidence of any ongoing major mergers or significant tidal disturbances affecting the main body of the galaxy, but possible minor disturbances can not be ruled out.
