The galaxy presents as a relatively smooth, elliptical-like structure, with a high degree of central concentration. The galaxy exhibits a dominant spheroidal component, with a distinct lack of discernible spiral arms or a prominent disk. Its overall shape is mostly round. There may be some minor disturbance in its structure but appears to be a relatively isolated system. The galaxy's color profile indicates a population of older stars, as evidenced by the redder hue of the central bulge and the slightly bluer outer regions. The redder central region suggests a greater density of older, redder stars, while the slightly bluer halo may indicate ongoing, but subdued, star formation in the outer regions. The galaxy appears to be a mature system with a considerable stellar mass. Star formation is likely occurring at a relatively low rate, and the galaxy is likely dominated by an older stellar population. 
