The galaxy presents as a relatively smooth, elliptical-like structure. Its color exhibits a pronounced yellowish hue, suggesting a dominant population of older stars and a lack of significant ongoing star formation. The galaxy appears fairly rounded, with a generally symmetrical morphology and no obvious spiral arms or bar-like features. There are no visible signs of recent or ongoing major merger events; the galaxy seems largely undisturbed. The central region is slightly brighter, indicating a concentration of stellar density, possibly a galactic bulge. The overall appearance suggests a passively evolving system likely composed mostly of Population II stars.
