The galaxy presents as a somewhat symmetrical, elliptical-like structure. It appears to be a fairly large galaxy given its brightness and spatial extent. The central bulge is a dominant feature, exhibiting a concentrated luminosity, suggestive of an older stellar population. The primary color of the bulge appears to be yellowish. This color may indicate an older stellar population consisting of less massive stars. There is evidence of a surrounding disk or halo, but the structure is less defined than the central bulge. The outer regions display a bluer tint, hinting at the presence of younger stars and some ongoing star formation, but the star formation rate seems relatively low. There are no obvious signs of significant disturbance such as tidal tails or strong asymmetries, suggesting that the galaxy is relatively undisturbed. A high percentage of its mass is in the form of stars.
