The galaxy appears to be a relatively luminous object at a moderate redshift, indicating a significant distance. Its morphology is generally smooth and spheroid-like, suggesting it may be an elliptical galaxy or a lenticular galaxy seen at a relatively low inclination. There is some evidence of a disk-like structure, which is not well defined, which further suggest it might be a lenticular galaxy with a dim disk.

The color is relatively red, which could mean it has a low rate of star formation and is primarily composed of older stars. However, the overall luminosity indicates there is likely still significant activity within the galaxy, and this could also be due to dust obscuration within the system. While not showing any evidence of major mergers, the overall structure looks slightly asymmetric, potentially hinting at past minor disturbances or interactions with other galaxies.
