The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a bright, concentrated central bulge, surrounded by a fainter, more diffuse halo. The core displays a yellowish hue, suggesting an older stellar population. Moving outward, the galaxy exhibits a subtle color gradient towards bluer tones. The morphology suggests that it is not an actively merging system. However, there is some indication of minor asymmetry or perturbation. Overall, this galaxy appears to be a well-evolved system with moderate mass and a suppressed star formation rate.