The galaxy presents an elliptical morphology with a moderate degree of elongation. Its central region displays a yellowish-white hue, suggesting a substantial population of older stars. Surrounding this core, there is a faint bluish-green halo, potentially indicating the presence of younger stellar populations and ongoing star formation, although not particularly vigorous. The galaxy lacks any visible spiral arm structure or a well-defined disk. Its overall appearance is relatively smooth, with no apparent signs of significant mergers or tidal disturbances, which suggests it has undergone relatively stable evolution recently.
