The galaxy presents as a centrally concentrated object with a generally smooth morphology, exhibiting a high degree of radial symmetry. There is little to no evidence of spiral arm structure or a distinct disk component. The light profile is generally smooth and decreases gradually with radial distance from the center. The galaxy is primarily composed of a singular, symmetrical, unresolved bulge. The color gradient indicates a core that is moderately redder than the outer regions, suggesting a difference in stellar population or dust content. The apparent ellipticity is low, tending toward a circular appearance. There is no evidence of tidal features, major mergers, or other significant disturbances in the galaxy's structure.
