The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The overall light distribution appears spheroidal, lacking prominent spiral arms or a well-defined disk. There is an absence of significant dust lanes or knotty, irregular structures usually associated with ongoing star formation. The galaxy exhibits a slight colour gradient from the core outwards, transitioning towards a redder colour. There is no obvious indication of any major mergers. There are some possible minor disturbances but they are not obvious.
