The galaxy presents as an elongated structure, indicating a likely elliptical morphology or a disk galaxy viewed at a high inclination. The light distribution is relatively smooth, with a higher concentration of light in the center. The galaxy exhibits a redder color profile in the center, suggesting an older stellar population dominating the core, whereas the bluer light is more broadly distributed across the galaxy, suggesting more star formation activity in those areas. There is evidence of a possible interaction or minor disturbance as shown by the distortion of the light in the upper region of the galaxy. Overall, the galaxy is relatively compact in appearance.
