The galaxy presents a predominantly smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, surrounded by a more diffuse halo. The galaxy exhibits a relatively high degree of rotational symmetry and appears somewhat flattened. There is a hint of disk structure with evidence of some features in the halo region but no strong spiral arm or bar are visible. Redder hues appear in the outer regions, possibly indicative of an older stellar population with minimal active star formation. Overall, the galaxy exhibits a mature and evolved form.
