This galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population likely dominates the core. The surrounding region displays a more diffuse, bluish glow, possibly indicating the presence of a younger stellar population and ongoing, though perhaps limited, star formation in the outer regions. While no distinct spiral arms or bar features are discernible, a slight asymmetry in the outer isophotes may suggest minor gravitational interaction or past merger event. The galaxy appears somewhat round, exhibiting a moderate degree of ellipticity, and possesses a substantial mass. Overall, this galaxy is consistent with a transitional object, displaying characteristics of both early-type and late-type systems.
