The galaxy appears to be an elliptical type, displaying a generally smooth and concentrated morphology. There is a central bulge that is slightly elongated, not perfectly spherical. The light distribution appears to be quite even, with no obvious spiral arm structures or significant dust lanes visible in this image. The galaxy has a noticeable red hue, likely indicating an older stellar population with lower rates of current star formation. There is a slight hint of possible tidal disturbances or minor interactions, but overall, the galaxy's structure seems relatively undisturbed.
