The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its overall shape appears to be elongated, displaying a cigar-like appearance. There is little evidence of spiral arm structure or distinct features that would indicate a disk component. The light distribution is relatively uniform, with a gradual decrease in intensity from the center outwards. No significant dust lanes or star-forming regions are apparent, suggesting a low rate of current star formation. There are no obvious signs of recent or ongoing merger activity or gravitational disturbance. The galaxy has a moderate redshift, indicating that it is located at a considerable distance. The color suggests an older stellar population, with a yellow-red hue dominating the galaxy's overall light.
