This galaxy presents as an elliptical or lenticular type. Its overall shape is largely smooth and rounded, exhibiting a high degree of central concentration. The core is bright and appears yellowish/orange in color, suggesting a population of older stars. There may be a slight hint of a disk structure surrounding the core, although this is not well-defined. There is no evidence of spiral arms or significant dust lanes within the galaxy's structure, which are consistent with a galaxy that has largely ceased active star formation. No signs of any major mergers or significant disturbances.
