The galaxy appears to be a spheroidal system with a smooth, centralized concentration of light. The object exhibits a relatively round morphology, lacking any discernible spiral arms or a prominent disk structure. A gradual decrease in luminosity is observed moving outwards from the core, suggesting a fairly even distribution of stellar populations or a lack of significant dust extinction. The core itself displays a yellowish-white hue. The outer regions appear to be undergoing minimal active star formation. Evident based on a lack of distinct blue regions. No signs of ongoing major merger events or tidal disturbances are noted. 
