The galaxy presents as a relatively smooth, elliptical-like object. Its core is a bright, concentrated yellowish-white, with the intensity diminishing gradually outwards. There is a minimal presence of distinct spiral arms or substructure visible. The object is generally rounded. The galaxy displays no clear signs of ongoing merging activity or major disturbances to its overall structure; it appears to be a fairly settled system. The color suggests a population of older stars, indicating a relatively low rate of star formation.
