This galaxy presents as a relatively smooth, single object with minimal discernable structure. It exhibits a bright, concentrated central bulge that transitions into a more diffuse halo or disk. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, possibly indicating a lack of significant recent star formation. There is a slight hint of bluer colors in the outer regions, though subdued, which might suggest some low-level ongoing star formation. The overall morphology is elliptical, with no clear evidence of spiral arms or a bar structure. There is no obvious sign of any major merger events or strong tidal disturbances, although minor interactions cannot be ruled out. Based on its size and brightness, this galaxy likely possesses a substantial mass.
