The galaxy presents a primarily smooth and rounded morphology, with a high degree of central concentration indicated by a bright, yellowish core. The overall color suggests an evolved stellar population. Faint blue regions appear in the outer regions, possibly indicative of some ongoing, low-level star formation activity. There is no strong evidence of spiral arm structure or significant tidal disturbances. The shape is generally elliptical, with minimal deviation from a perfectly round profile. The structure appears largely undisturbed, suggesting it is not currently undergoing a major merging event. 
