The galaxy presents as a relatively smooth, elliptical object, appearing mostly round. Its core is intensely luminous, displaying a yellowish-white hue, suggesting an older stellar population dominating the central region. Moving outwards from the core, the galaxy exhibits a gradual decrease in surface brightness. The surrounding halo is less defined and shows a reddish tint, possibly indicating the presence of some dust or a population of older, redder stars. There is no clear evidence of spiral arms or a defined disk structure. The galaxy appears generally undisturbed, showing no major signs of ongoing mergers or tidal interactions. Faint irregularities may be present, but overall, the galaxy maintains a fairly uniform and relaxed morphology.
