The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology with a high degree of central concentration. The light distribution suggests a generally ellipsoidal shape, appearing nearly round. The color gradient transitions from a bright, yellowish-white core to a slightly redder halo. There are no apparent spiral arms, dust lanes, or other features indicative of recent or ongoing star formation. The overall structure suggests a relatively old stellar population, consistent with a galaxy that has largely exhausted its gas supply. There is no obvious sign of a major ongoing merger event, or any significant gravitational disturbances.
