The galaxy appears as a centrally concentrated, elliptical-like structure. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the galaxy gradually fades into a bluish halo, possibly indicating the presence of younger, bluer stars in its outer regions. The overall morphology is smooth, with no discernible spiral arms or distinct features of disturbance. The observed color gradient, from yellow to blue moving outward, might indicate radial differences in stellar population ages or metallicity. 
