The galaxy presents a predominantly smooth morphology, appearing elliptical in shape. The light distribution suggests a concentration towards the center, indicative of a significant bulge component. There is a subtle elongation, but no spiral arm structure is clearly discernible in this image. The galaxy has a redder color, suggesting an older stellar population and a lower rate of current star formation. Faint, extended emission is present, forming a halo-like structure around the central region. There might be the faintest hint of disturbance in its morphology, but it is too subtle to be considered a merger remnant.
