The galaxy appears to be a relatively smooth, elliptical system. It presents a concentrated central bulge that gradually fades outward without any distinct spiral arm structure. The light distribution suggests that the galaxy is dominated by an older stellar population, which is consistent with its reddish-yellow color, although it does contain some bluer light as well. The overall form is neither perfectly spherical nor highly elongated, leaning more towards an intermediate ellipticity. There are no obvious signs of active merging or significant tidal disturbances affecting its morphology.
