The galaxy presents as a slightly elongated, yellow-hued spheroid. A central, bright bulge dominates the structure. Surrounding the bulge is a fainter, more diffuse halo. The color gradient from the center to the outer regions suggests an aging stellar population and a relatively low star formation rate. There may be faint, diffuse spiral arm-like structures, but these features are not well-defined. Overall, the galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major merger events. The roundness of the spheroid suggests it is not completely face on, but closer to that orientation than edge on. It is likely that this galaxy is an early-type spiral galaxy.
