The galaxy appears as a relatively smooth, elliptical-like structure. The light distribution is concentrated toward the center, with a gradual decrease in intensity moving outwards. There is a dominant central bulge, a dense concentration of stars. The galaxy exhibits a yellowish hue, suggestive of an older stellar population. No distinct spiral arms or significant dust lanes are visible. There is a faint outer halo surrounding the central region, and no major or minor disturbances are detected. The shape is roughly circular, with minimal elongation or distortion, but it appears to be slightly oblate rather than perfectly spherical.
