The galaxy presents as a predominantly smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing bright and yellowish. The light gradually diffuses outwards, forming a halo. This halo appears slightly more flattened than perfectly circular. Faint tendrils or extensions emerge from the outer halo, suggesting possible minor gravitational disturbances or interactions, though the overall structure is not significantly disrupted. There is very little evidence of spiral arm structure. The color suggests an older stellar population within the galaxy.
