The galaxy appears to be an elliptical galaxy, with a smooth, concentrated central bulge that emits light at shorter wavelengths, shown through its yellow color. The galaxy shows a nearly perfect circular shape, with a slight extension in the horizontal direction. It presents no obvious spiral arm structures or evidence of active star formation regions. The smooth, diffuse halo is a combination of shorter and longer wavelengths of light, depicted through the mixture of red, green, and blue. There is no significant dust lane or obscuration visible. The galaxy exhibits a relatively symmetrical morphology, without prominent tidal tails or distortions, and no clear indication of recent major merger events. It would be beneficial to further investigate the luminosity profile, to better constrain its morphology and formation history.
