The galaxy presents a smooth, centrally concentrated morphology, appearing largely elliptical in shape. Its core exhibits a bright, orange-yellow hue, suggesting an older stellar population, potentially dominated by red giant and red dwarf stars. The light smoothly diffuses outwards from the core, with a slight reddening towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes visible within the galaxy’s profile. The absence of blue light suggests little ongoing star formation. Overall, it presents the characteristics of a relatively quiescent, evolved galaxy.
