The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. Moving outward from the core, the color shifts to a more diffuse, slightly bluer tone. This implies the presence of some younger, bluer stars in the outer regions, possibly indicating ongoing, but relatively low, star formation activity. There is no clear evidence of spiral arms or a well-defined disk structure; instead, it appears to be an amorphous object that appears to be isolated, with no obvious signs of major tidal disturbances or interactions with nearby galaxies, although very faint disturbances can be seen. The overall morphology leans toward an elliptical galaxy at a moderate redshift.
