The galaxy presents an overall elliptical morphology, appearing smooth in structure with no readily discernible spiral arms or bar. The light distribution suggests a relatively uniform stellar population. There is a slight elongation in the structure, hinting at a possible transition between spherical and more cigar-shaped form. A redder central region may indicate an older stellar population concentration or a higher dust content within the core. There appears to be no signs of recent major merger activity, though minor tidal disturbances cannot be ruled out based on the image's resolution. The galaxy displays a moderate redshift, indicating a significant distance and lookback time. Overall, this galaxy appears to be a typical elliptical galaxy.
