The galaxy presents as a generally smooth, elliptical structure with a high degree of central concentration. It exhibits a dominant, centrally located bulge that appears nearly spherical. The light distribution is relatively uniform throughout the visible body, with a noticeable gradient in color, shifting from a yellowish hue at its core to a slightly redder tint at its outer edges. There is little evidence of significant star formation activity; the overall color suggests an older stellar population. No prominent spiral arms or distinct features like dust lanes are visible. The morphology suggests that the galaxy is relatively undisturbed, likely having undergone significant relaxation and homogenization of its stellar distribution. There may be some indication of tidal distortion that needs to be examined further with other observations.
