The galaxy presents as a slightly elongated spheroid with a moderately concentrated core. A faint halo surrounds the central region, exhibiting a diffuse and somewhat irregular morphology. The overall color gradient indicates bluer hues in the outer regions, transitioning to redder tones towards the core, suggesting potential variations in stellar populations or dust content. There is little evidence of distinct spiral arms or other prominent features characteristic of disk galaxies. The general appearance suggests a galaxy that is either an elliptical or a lenticular galaxy, with a relatively smooth distribution of light.
