The galaxy presents a generally smooth morphology. It exhibits a somewhat elliptical shape, appearing mostly round. There is a central bulge region with a higher concentration of luminosity that gradually decreases outward. Faint traces of a disk structure seem to be present in the outer regions, but they are not sharply defined. There is no obvious sign of strong spiral arm features or active star-forming regions. No major disturbances are seen in the overall structure, indicating that it is most likely not undergoing a major merger. There may be slight evidence of a minor disturbance. Its color suggests an older stellar population, with a redshift measurement indicating it is at a relatively moderate distance.
