The galaxy presents an elliptical morphology, appearing mostly smooth and spheroidal in structure. A bright, concentrated central bulge is visible, showing a yellowish-white hue. The galaxy's color profile suggests an older stellar population. A faint disk-like component is present but poorly defined, and no significant spiral arms are visible. The galaxy exhibits a relatively high degree of roundness. There is no clear evidence of any ongoing major merging events or strong tidal disturbances affecting the morphology. The overall form suggests that this is a mature galaxy with a subdued star formation rate.
