The galaxy presents as a smooth, elliptical structure with a bright, concentrated central bulge. The overall color profile suggests a relatively old stellar population, with a yellowish hue dominating the core. The outer regions exhibit a fainter, more diffuse glow, transitioning gradually from the central brightness. No distinct spiral arms or strong dust lanes are evident. There appears to be a slight elongation along one axis, deviating from a perfectly circular shape. The galaxy exhibits minimal signs of ongoing star formation, with a lack of prominent blue regions typically associated with young, hot stars. There is no strong evidence of any major ongoing mergers or tidal disturbances, although a subtle asymmetry might suggest past gravitational interactions. The overall morphology suggests a system nearing the end of its star-forming lifecycle.
